== �--== -=--=- �=------===--====-==-=--=-=-==- __;;;;._ ____________ _ RESEARCH TRIANGLE INSTITUTE /RTI Contract No ■- FO4703-91-C-0112 RTI Report No. RTl/5180/77-43F September 10, 1996 Modeling Unlikely Space-Booster Failures in Risk Calculations 19961025 122 Final Report Prepared for Department of the Air Force 45th Space Wing (AFSPC) Safety Office - 45 SW/SE Patrick AFB, FL 32925 and Department of the Air Force 30th Space Wing (AFSPC) Safety Office- 30 SW/SE Vandenberg AFB, CA 93437 Distribution authorized to US Government agencies and their contractors to protect administrative/ operational use data, 10 September 96. Other requests for this document shall be referred to the 30th Space Wing (AFSPC) Safety Office (30 SW/SE), Vandenberg AFB, CA 93437, or 45th Space Wing (AFSPC) Safety Office (45 SW/SE), Patrick AFB, FL 32925. 'mJC QUALITY INSPECTED ff 3000 N. Al1antic Avenue • Cocoa Beach, Flo0ida 329315029 US/1 ^03b0^-^~/a C ontract No. FO4703-91-C -0112 Task No. 10/95-77, Subtask 2.0 RTI Report No. RTI/5180/77-43F September 10,1996 Modeling Unlikely Space-Booster Failures in Risk Calculations Final Report Prepared by James A . W ard, Jr. Robert M . M ontgomery of Research Triangle Institute C enter for A erospace Technology Launch Systems Safety D epartment Prepared for D epartment of the A ir Force 45th Space W ing (A FSPC ) Safety Office-45 SW /SE Patrick A FB, FL 32925 and D epartment of the A ir Force 30th Space W ing (A FSPC ) Safety Office-30 SW /SE Vandenberg A FB, C A 93437 Distribution authorized to US G overnment agencies and their contractors to protect administrative/ operational use data, 10 September 96. Other requests for this document shall be referred to the 30th Space Wing (AFSPC ) Safety Office (30 SW/SE), Vandenberg AFB , C A 93437, or 45th Space Wing (AFSPC ) Safety Office (45 SW/SE), Patrick AFB , FL 32925. NSN 7540-01-280-5 500 Standard Form 298 (Rev. 2-89) REPO RT DO CUM ENTATIO N PAGE form Approved 0MB No, 0704-0188 Public reporting burden for this collection of information is estimated to average 1 hour per response, including the time for reviewing instructions, searching existing data sources, gathering and maintaining the data needed, and completing and reviewing the collection of information. Send comments regarding this burden estimate or any other aspect of this collection of information, including suggestions for reducing this burden, to Washington H eadquarters Services, D irectorate for Information Operations and Reports, 1215 J efferson D avis H ighway, Suite 1204, Arlington, VA 22202-4302, and to the Office of Management and Budget, Paperwork Reduction Project (0704-0188), Washington, D C 20503. AG E NC Y USE O NLY (Leave blank) 2. RE PO RT DATE September 10,1996 3 . RE PO RT TYPE AND DATE S C O VE RE D Final 4. TITLE AND SUBTITLE Modeling Unlikely Space-Booster Failures in Risk Calculations 5. FUNDING NUMBE RS C: FO4703-91-C-0112 TA: 10/95-77 6. AUTHO R(S) J ames A. Ward, J r. Robert M. Montgomery 7. PE RFO RMING O RG ANIZATIO N NAME (S) AND ADDRE SS(E S) Research Triangle Institute * ACTA, Inc.** 3000 N. Atlantic Avenue Skypark3 Cocoa Beach, FL 32931 23430 H awthorne Blvd., Suite 300 Torrance, CA 90505 8. PE RFO RMING O RG ANIZATIO N RE PO RT NUMBE R RTI/5180/77-43F 9. SPO NSO RING /MO NITO RING AG E NC Y NAME (S) AND ADDRE SS(E S) D epartment of the Air Force (AFSPC) D epartment of the Air Force (AFSPC) 30th Space Wing 45th Space Wing Vandenberg AFB, CA 93437 Patrick AFB, FL 32925 Mr. Martin Kinna (30 SW/SEY) L ouis J . Ullian, J r. (45 SW/SED ) 10. SPO NSO RING /MO NITO RING AG E NC Y RE PO RT NUMBE R 11. SUPPLE ME NTARY NO TE S * Subcontractor ** Prime Contractor 12a. DISTRIBUTIO N/AVAILABILITY STATE ME NT D istribution authorized to US Government agencies and their contractors to protect administrative/operational use data, 10 September 96 . Other requests for this document shall be referred to the 30th Space Wing (AFSPC) Safety Office (30 SW/SE),Vandenberg AFB, CA 93437, or 45th Space Wing (AFSPC) Safety Office (45 SW/SE), Patrick AFB, FL 32925. 12b. DISTRIBUTIO N C O DE 13 . ABSTRAC T (Maximum 200 words) Missile and space-vehicle performance histories contain many examples of failures that cause, or have the potential to cause, significant vehicle deviations from the intended flight line. In RTI’s risk-analysis program, D AMP, such failures are referred to as Mode-5 failure responses. Although Mode-5 failure responses are much less likely to occur than those that result in impacts near the flight line, risk-analysis studies are incomplete without them. This report shows how impacts from Mode-5 failures are modeled in program D AMP. The impact density function used for this purpose contains two shaping constants that control the rate at which the density function drops in value as the angular deviation from the flight line and the impact range increase. Certain Mode-5 malfunctions are simulated, and the two shaping constants then chosen by trial and error so that impacts from the simulated malfunctions and the theoretical density function are in close agreement. An appendix to the report contains a listing and brief narrative failure history of the Atlas, D elta, and Titan missile and space-vehicle launches from the Eastern and Western Ranges from the beginning of each program through August 1996 . Each entry gives the vehicle configuration, whether the flight was a success, the flight phase in which any anomalous behavior occurred, and a classification of vehicle behavior in accordance with defined failure-response modes. 14. SUBJE C T TE RMS launch risk, unlikely failure modeling, booster failure probabilities 15. NUMBE R O F PAG E S 180 16. PRIC E C O DE 17. SE C URITY C LASSIFIC ATIO N O F RE PO RT Unclassified 18. SE C URITY C LASSIFIC ATIO N O F THIS PAG E J nclassified 19, SE C URITY C LASSIFIC ATIO N O F ABSTRAC T J nclassified 20. LIMITATIO N O F ABSTRAC T SAR Prescribes by ANSI Std. £39-18 298-102 A bstract M issile and space-vehicle performance histories contain many examples of failures that cause, or have the potential to cause, significant vehicle deviations from the intended flight line. In RTFs risk-analysis program, D A M P, such failures are referred to as M ode-5 failure responses. A lthough M ode-5 failure responses are much less likely to occur than those that result in impacts near the flight line, risk-analysis studies are incomplete without them. This report shows how impacts from M ode-5 failures are modeled in program D A M P. The impact density function used for this purpose contains two shaping constants that control the rate at which the density function drops in value as the angular deviation from the flight line and the impact range increase. C ertain M ode-5 malfunctions are simulated, and the two shaping constants then chosen by trial and error so that impacts from the simulated malfunctions and the theoretical density function are in close agreement. A n appendix to the report contains a listing and brief narrative failure history of the A tlas, D elta, and Titan missile and space-vehicle launches from the Eastern and W estern Ranges from the beginning of each program through A ugust 1996. Each entry gives the vehicle configuration, whether the flight was a success, the flight phase in which any anomalous behavior occurred, and a classification of vehicle behavior in accordance with defined failure-response modes. Various filtering or data weighting techniques are described. The empirical data are then filtered to estimate (1) failure probabilities for A tlas, D elta, and Titan, and (2) percentages of future failures that will result in M ode-5 (and other M ode) responses. 9/10/96 i RTI Table of C ontents 1. Introduction............................... 1 2. Examples Showing Need for M ode 5..........................................................................................3 3. U nderstanding the M ode-5 Failure Response..........................................................................7 3.1 Effects of M ode-5 Shaping C onstants...................... 9 3.2 Effects of Shaping C onstant on D A M P Results........................... 9 4. M ethodology for A ssessing Failure Probabilities..................................................................13 4.1 The Parts-A nalysis A pproach.................................. 13­ 4.2 The Empirical A pproach............................................. 15 5. C omputation of Failure Probabilities.......................................... 16 5.1 Overall Failure Probability....................................... 16 5.2 Relative and A bsolute Probabilities for Response M odes..........................................24 5.3 Relative Probability of Tumble for Response-M odes 3 and 4...................................30 6. Shaping C onstants Through Simulation............................................................. 31 6.1 M alfunction Turn Simulations................................................ 31 6.1.1 Random-A ttitude Failures..... ....................................................................31 6.1.2 Slow-Tum Failures.................................................. 32 6.1.3 Factors A ffecting M alfunction-Turn Results.....................................................33 6.1.4 M alfunction-Turn Results for A tlas H A S.............................................................35 6.2 Shaping C onstants for A tlas H A S.....................................................................................37 6.2.1 Optimum M ode-5 Shaping C onstants.................................................................37 6.2.2 Launch-A rea M ode-5 Risks................. ......49 6.2.3 Effects of M ode-5 C onstants on Ship-H it C ontours..........................................51 6.2.4 Range D istributions of Theoretical and Simulated Impacts...........................58 6.3 Shaping C onstants for D elta-G EM .......................... 60 6.3.1 Optimum M ode-5 Shaping C onstants................................ 61 6.3.2 Launch-A rea M ode-5 Risks........................................ 64 6.4 Shaping C onstants for Titan IV............................................................. 65 6.5 Shaping C onstants for ELV1................................................................ 69 6.6 Shaping C onstants for Other Launch Vehicles..............................................................72 7. Potential Future Investigations............................................................................ 73 8. Summary............................................... 74 9/10/96 ii RTI A ppendix A . Failure Response M odes in Program D A M P....................................................79 A ppendix B. Shaping-C onstant Effects on M ode-5 Impact D istributions...........................81 A ppendix C . Filter C haracteristics............................................................... ...90 A ppendix D . Launch and Performance H istories......................................................................96 D .l Basic D ata............................................... 96 D .l.l D ata Sources...................................... 96 D .1.2 A ssignment of Failure-Response M odes......................... 98 D .1.3 A ssignment of Flight Phase............................ 98 D .1.4 Representative C onfigurations............................. 100 D .2 A tlas Launch and Performance H istory.......................................................................101 D .2.1 A tlas Launch H istory.............................................................................................103 D .2.2 A tlas Failure Narratives........................................................................................115 D .3 D elta Launch and Performance H istory................................... 133 D .3.1 D elta Launch H istory................................. 136 D .3.2 D elta Failure Narratives..................................................................................... 142 D .4 Titan Launch and Performance H istory................................................. 146 D .4.1 Titan Launch H istory..............................................................................................149 D .4.2 Titan Failure Narratives.............................. 157 D .5 Thor Launch and Performance H istory (Not Including D elta).............................164 D .5.1 Thor and Thor-Boosted Launch H istory...........................................................164 D .5.2 Thor and Thor-Boosted Failure Narratives..................................... 167 References.......................... 171 9/10/96 iii RTI Table of Figures Figure 1. Joust Impact Trace Showing a M ode-5 Failure Response........................................6 Figure 2. A tlas H A S Risk C ontours for Inner-Ear Injury with A = 3.0..................................11 Figure 3. A tlas IIA S Risk C ontours for Inner-Ear Injury with A = 3.5..................................12 Figure 4. Filter Factor Results for Representative C onfigurations of A tlas........................23 Figure 5. C ombined Random-A ttitude and Slow-Turn Results...................... 36 Figure 6. A tlas IIA S Breakup Percentages for Random-A ttitude Turns..............................37 Figure 7. A tlas IIA S Impacts with No Breakup................................................... 39 Figure 8. A tlas IIA S Impacts with Breakup..................................................................................40 Figure 9. A tlas IIA S Simulation Results with B = 1,000..................... 42 Figure 10. A tlas IIA S Simulation Results with B = 50,000....................................................... 44 Figure 11. A tlas H A S Simulation Results with B = 100,000..................................................... 45 Figure 12. A tlas IIA S Simulation Results with B = 500,000..................................................... 46 Figure 13. A tlas IIA S Simulation Results with B = 5,000,000..................................................47 Figure 14. Effects of Breakup q-alpha on A for A tlas IIA S....................................................49 Figure 15. M ode-5 D ensity-Function Values at Three M iles.................................................51 Figure 16. A tlas H A S M ode-5 Ship-H it C ontours with A = 3.00..........................................53 Figure 17. A tlas H A S A ll-M o'de Ship-H it C ontours with A = 3.00............... .54 Figure 18. A tlas IIA S M ode-5 Ship-H it C ontours with A = 3.45..........................................55 Figure 19. A tlas IIA S A ll-M ode Ship-H it C ontours with A = 3.45.......................................56 Figure 20. A tlas IIA S M ode-5 Ship-H it C ontours with A = 6.30..........................................57 Figure 21. A tlas IIA S A ll-M ode Ship-H it C ontours with A = 6.30.......................................58 Figure 22. Impact-Range D istributions.......................... 59 Figure 23. D elta-G EM Breakup Percentages................................................................................61 Figure 24. D elta-G EM Simulation Results with B —1,000......................................................62 Figure 25. D elta-G EM Simulation Results with Best-Fit Shaping C onstants......................... 63 Figure 26. Titan TV Breakup Percentages....................................................................................65 Figure 27. Titan Simulation Results with B = 1,000........................ 66 Figure 28. Titan Simulation Results with Best-Fit Shaping C onstants................................67 Figure 29. LLV1 Breakup Percentages.................................................. 69 Figure 30. LLV1 Simulation Results with B = 1,000..................................................... 70 9/10/96 iv RTI Figure 31. LLV1 Simulation Results with Best-Fit Shaping C onstants.................................71 Figure 32. f-Ratios for Ranges from 1 to 25 M iles......................................................................86 Figure 33. Percentage of Impacts Between Flight Line and A ny Radial.............................87 Figure 34. Percentage of Impacts in 5-D egree Sectors...............................................................88 Figure 35. Exponential W eights for Fading-M emory Filters..................................................93 Figure 36. Recursive Filter Factor for Last D ata Point...............................................................94 Figure 37; A tlas Launch Summary................................................................................................102 Figure 38. D elta Launch Summary.;..............................................................................................135 Figure 39. Titan Launch Summary....................................... 148 Figure 40. Thor Launch Summary................................................................................................164 Table of Tables Table 1. Effects of M ode-5 Shaping C onstant A on A tlas IIA Risks......................................10 Table 2. Predicted Failure Probabilities for Representative C onfigurations......................17 Table 3. Predicted Failure Probabilities for A ll C onfigurations............................................18 Table 4. C omparison of W eighting Percentages.........................................................................19 Table 5. Filter Factor Influence on W eighting Percentages......................................................21 Table 6. Failure Probabilities for A tlas, D elta, and Titan.........................................................24 Table 7. Number of A tlas Failures - A ll C onfigurations (532 Flights)..................................25 Table 8. Number of D elta Failures - A ll C onfigurations (232 Flights)..................................25 Table 9. Number of Titan Failures - A ll C onfigurations (337 Flights)..................................25 Table 10. Number of Eastern-Range Thor Failures (85 Flights).............................................25 Table 11. Number of Failures for A ll Vehicles (1186 Flights)................................................26 Table 12. D ate of M ost Recent Failure...........................................................................................26 Table 13. Percentage W eighting for Sample of 1186 Launches..............................................27 Table 14. Response-M ode Occurrence Percentages.................................................... 27 Table 15. Recommended Response-M ode Percentages for Flight Phases 0-2.................28 Table 16. Recommended Response-M ode Percentages for Flight Phases 0-1.................29 Table 17. A bsolute Failure Probabilities for Response M odes 1-5......................................29 Table 18. Percent of Response M odes 3 and 4 That Tumble....................................................30 9/10/96 v RTI Table 19. Sample Impact D istribution for A tlas H A S’with No Breakup.............................41 Table 20. Shaping C onstants for A tlas H A S..................................................................................48 Table 21. Shaping C onstants and Related Risks for A tlas ILA S'..............................................50 Table 22. Best-Fit C onditions for A tlas H A S.................................................. 52 Table 23. Shaping C onstants and Related Risks for D elta-G EM ............................................64 Table 24. Shaping C onstants for Titan IV.....................................................................................68 Table 25. Shaping C onstants for LLV1...........................................................................................72 Table 26. Summary of A Values for B = 1,000................... 72 Table 27. Failure Probabilities for A tlas, D elta, and Titan.......................................................75 Table 28. Recommended Response-M ode Percentages for Flight Phases 0 -2...................75- Table 29. Recommended Response-M ode Percentages for Flight Phases 0-1..................75 Table 30. A bsolute Failure Probabilities for Response M odes 1-5......................................76 Table 31. Summary of A Values for B = 1,000.......................................................................... 77 Table 32. Summary of Optimum M ode-5 Shaping C onstants................................................77 Table 33. Effect on f-Ratio of Varying M ode-5 C onstant A (B = 1000) - Part 1.................82 Table 34. Effect on f-Ratio of Varying M ode-5 C onstant A (B = 1000) - Part 2................83 Table 35. Effect on f-Ratio of Varying M ode-5 C onstant B (A = 3) - Part 1.......................84 Table 36. Effect on f-Ratio of Varying M ode-5 C onstant B (A = 3) - Part 2.......................85 Table 37. Filter A pplication for Failure Probability..................................................................95 Table 38. Flight-Phase D efinitions...................................................................................................99 Table 39. Flight Phases by Launch Vehicle..................................................................................99 Table 40. Summary of A tlas Vehicle C onfigurations..............................................................101 Table 41. A tlas Launch H istory.................................................................. 103 Table 42. Summary of D elta Vehicle C onfigurations..............................................................133 Table 43. D elta Launch H istory.....................................................................................................136 Table 44. Summary of Titan Vehicle C onfigurations..............................................................147 Table 45. Titan Launch H istory......................................................................................................149 Table 46. Thor Launch H istory....................................................................................... 165 9/10/96 vi RTI 1. Introduction The debris from most launch vehicles that fail catastrophically tend to impact close to the intended flight line. Typical failures that produce such results are premature thrust termination, stage ignition failure, tank rupture or explosion, or rapid out-of-control tumble. Less likely malfunctions may cause a vehicle to execute a sustained turn away from the flight line. Examples are control failures that cause the rocket engine to lock in a fixed position near null, or failures leading to erroneous orientation of the guidance platform. Such failures should not be ignored, since they may produce nearly all or a significant part of the risks to population centers that are more than a mile or so uprange or many miles away from the flight line. C onsequently, RTI has been tasked to estimate the probabilities of occurrence of these less-likely failures, and to determine optimum values for the shaping constants of the associated impact-density function. RU has developed a prototype risk-analysis program (1) to analyze the level of risk in the launch area when ballistic missiles and space vehicles are launched, and (2) to provide guidelines for launch operations and launch-area risk management. This program, "facility D A M age and Personnel injury" (D A M P), uses information about the launch vehicle, its trajectory and failure responses, and facilities and populations in the launch area to estimate hit probabilities and casualty expectations. W hen a missile or space vehicle malfunctions, people and facilities may be subjected to significant risks from falling inert debris, or from overpressures and secondary debris produced by a stage, component, or large propellant chunk that explodes on impact. A lthough fire, toxic materials, and radiation may also subject personnel to significant danger, these hazards are not addressed in program D A M P. H azards are greatest in the launch area and along the intended flight line, but lesser hazards exist throughout the area inside the impact limit lines. Small hazards exist even outside these lines if the flight termination system fails or other unlikely events occur. In computing launch-area risks, D A M P makes no attempt to model vehicle failures per se. A list of possible failures for any vehicle would be extensive, and variations in failures from vehicle to vehicle would complicate the modeling process. Instead, D A M P models failure responses. Regardless of the exact nature of the failures that can occur, there are only six possible response modes that affect risks on the ground, five for failure responses, and one to model the behavior of a normal vehicle. The six modes are described in A ppendix A . It can be seen from the descriptions that impacts resulting from failure-response M odes 1, 2, and 3 occur at most a mile or two from the launch point, while those from M ode 4 can only occur near the flight line, even though the vehicle may tumble before breakup or destruct. A lthough the hazards outside the launch area and away from the flight line may be small, vehicle flight tests through the years have demonstrated that finite hazards do exist in these areas. Such hazards are due almost entirely to M ode-5 failure responses, even through the probability of a M ode-5 failure may be only a small part of the total failure probability. The M ode-5 failure-response, theoretical though it is, was developed to reflect the facts that: (1) unlikely vehicle failures 9/10/96 1 RTI can cause impacts uprange or well away from the intended flight line, and (2) some vehicle failures cannot logically be classified as Response M odes 1,2,3, or 4. In keeping with the above, the M ode-5 impact-density function was developed with the characteristics listed below. The function, which fills the void left by M odes 1 through 4, is sufficiently robust to include all possible impacts, yet seemingly comports with observed test results. (1) Impacts can occur in any direction from the launch point and at any range within the vehicle's energy capabilities. (2) A t any given impact range from the launch point, the likelihood of impact decreases as the angular deviation from the flight line increases, becoming least likely in the uprange direction. For any fixed angular deviation from the flight line, the likelihood of impact decreases as the impact range increases. (3) A t fixed impact ranges near the launch point, the impact density function changes gradually as the impact direction swings 180° from downrange to uprange. A s the impact range increases, the decrease in the density function becomes progressively more and more rapid with change in impact direction. In other words, the greater the impact range, the more rapidly the density function changes with angular deviation from the flight line. A s modded in D A M P, the effects of destruct action on the M ode-5 density function are accounted for in the launch area by supplementing impacts inside the impact limit lines with those that would occur outside the impact limit lines if no destruct action were taken. The M ode-5 failure-response methodology was fully developed in an earlier RTI report111. A s pointed out there, the shape of the impact density function can be controlled somewhat through the selection of shaping constants that appear in the defining equation. Intuition suggests that the constants should be vehicle dependent, since (1) ruggedly built missiles would, after a malfunction, be more likely to impact well away from the flight line than would a fragile space vehicle that tends to break up before deviating significantly; and (2) certain vehicles, after a malfunction, tend to stabilize and continue thrusting at large angles of attack, while other vehicles that experience similar malfunctions tend to tumble. H it probabilities computed by program D A M P for targets located more than two miles or so uprange from the pad or more than a few miles from the flight line, are due almost entirely to the M ode-5 impact-density function. Thus, the assumed probability of occurrence of a M ode-5 response as well as the selected M ode-5 constants are of considerable importance. The tasking for this study is set forth as Task No. 10/95-77, Paragraph 2.0, of C ontract FO4703-91-C -0112. The primary purpose of the tasking is: "Perform a study to determine the best values for M ode-5 failure probability and the M ode-5 density­ function shaping constant A ." A lthough not explicitly included in the statement of work, the study also develops absolute failure probabilities for A tlas, D elta, and Titan, and 9/10/96 2 RTI relative probabilities of occurrence for all failure-response modes for these vehicles, LLV1, and other new launch systems. A lthough it may be reasonable to establish the relative probability of occurrence of a M ode-5 failure response by empirical means, the number of M ode-5 failures is too small to have any hope of establishing accurate values for the shaping constants from this sample alone. Inadequate descriptions of vehicle behavior in the available historical records and uncertainty in impact location following a malfunction add to the difficulty of classifying failure responses. In view of the limited data available for vehicles that have experienced M ode-5 failures, the values chosen for the M ode-5 constants must depend on simulations of vehicle behavior following failure. 2. E xamples Showing Need for Mode 5 The need for a M ode-5 response or some similar response mode (or a multiplicity of other response modes) can be seen from the following vehicle performance descriptions extracted from A ppendix D : (1) A tlas 8E, 24 Jan 61. M issile stability was lost at about 161 seconds, some 30 seconds after BEC O, probably due to failure of the servo-amplifier power supply. The sustainer engine shut down at 248 seconds, and the vernier engines about 10 seconds later. Impact occurred 1316 miles downrange and 215 miles crossrange. (2) Titan M -4,6 Oct 61. A one-bit error in the W velocity accumulation caused impact 86 miles short and 14 miles right of target. (3) A tlas 145D (M ariner R-l), 22 July 62. Booster stage and flight appeared normal until after booster staging at guidance enable at about 157 seconds. Operation of guidance rate beacon was intermittent. D ue to this and faulty guidance equations, erroneous guidance commands were given based on invalid rate data. Vehicle deviations became evident at 172 seconds and continued throughout flight with a maximum yaw deviation of 60° and pitch deviation of 28° occurring at 270 seconds. The vehicle deviated grossly from the planned trajectory in azimuth and velocity, and executed abnormal maneuvers in pitch and yaw. The missile was destroyed by the RSO at 293.5 seconds, some 12 seconds after SEC O. (4) A tlas SLV-3 (G TA -9), 17 M ay 66. Vehicle became unstable when B2 pitch control was lost at 121 seconds. Loss of pitch control resulted in a pitch-down maneuver much greater than 90°. G uidance control was lost at 132 seconds. A fter BEC O, the vehicle stabilized in an abnormal attitude. A lthough the vehicle did not follow the planned trajectory, SEC O (at 280 seconds), VEC O (at 298 seconds), and A gena separation occurred normally from programmer commands. (5) A tlas 95F (A BRES/A FSC ), 3 M ay 68. Immediately after liftoff the telemetered roll and yaw rates indicated that the missile was erratic. D uring the first 10 seconds of flight the missile yawed hard to the left. It then began a hard yaw to the right, 9/10/96 3 RTI crossed over the flight line and continued toward the right destruct line. Shortly thereafter the missile apparently pitched up violently and the IIP began moving back toward the beach. The missile was destructed at about 45 seconds when the altitude was about 14,000 feet and the downrange distance about 9 miles. M ajor pieces impacted less than a mile offshore, indicating uprange movement of the impact point during the last part of thrusting flight. (6) D elta Intelsat III, 18 Sep 68. D ue to loss of rate gyro, undamped pitch oscillations began at 20 seconds. A series of violent maneuvers followed at 59 seconds. D uring the 13-second period while these maneuvers continued, the vehicle pitched down some 270°, then up 210°, and then made a large yaw to the left. A t 72 seconds the vehicle regained control and flew stably in a down and leftward direction until 100 seconds. A t this time, with the main engine against the pitch and yaw stops, the destabilizing aerodynamic forces became so' large that quasi­ control could no longer be maintained. The first stage broke up at 103 seconds. The second stage was destroyed by the RSO at 110.6 seconds. M ajor pieces impacted about 12 miles downrange and 2 miles left of the flight line. (7) D elta Pioneer E, 27 A ug 69. First-stage hydraulics system failed a few seconds before first-stage burnout (M EC O). The vehicle pitched down, yawed left, rolled counterclockwise driving all gyros off limits, and then tumbled. Second-stage separation and ignition occurred while the vehicle was out of control. A fter about 20 seconds, the second stage regained control in a yaw-right, pitch-up attitude. It flew stably in this attitude for about 240 seconds until destroyed by the safety officer at T+484 seconds. (8) A tlas 68E, 8 D ec 80. Flight appeared normal until 102.7 seconds when the lube oil pressure on the B2 booster engine suddenly dropped. A t 120.1 seconds, the engine shut down, followed 385 msec later by guidance shutdown of the Bl engine. The asymmetric thrust during shutdown caused yaw and roll rates that the flight control system could not correct. A s a result, attitude control was lost and the thrusting sustainer pivoted the missile to a retrofire attitude before the vehicle could be stabilized. A fter the booster package was jettisoned, the missile was stabilized and decelerating in the retrofire mode by 148 seconds. The sustainer continued thrusting in this attitude until 282.9 seconds when reentry heating apparently caused sustainer shutdown and vehicle breakup. 9/10/96 4 RTI It is obvious from the response-mode definitions in A ppendix A that none of the described vehicle failures can be considered as a M ode 1, 2, or 3 response, or a M ode-4 on-trajectory failure.* Except possibly for (2), it also seems apparent that none can be modeled as either a rapid tumble or a slow turn. * Although prompt destruct action during any of the described flights might have resulted in a Mode-4 classification, the safety officer typically needs several seconds to evaluate data after a malfunction. Quick action is contrary to safety philosophy if impact limit lines are not threatened and the destruct system is not at risk, since additional flight time enhances the user's opportunity to pinpoint the nature of the problem. 9/10/96 5 RTI A good illustration of a M ode-5 failure response occurred during launch of Prospector (Joust) on the Eastern Range in June 1991. The Joust consists of a single-stage C astor IV-A solid-propellant rocket motor and a payload module. The "vehicle made a radical pitch-up maneuver due to- aft-skirt structural failure at approximately T+14 Seconds." 121 The vacuum instantaneous impact trace from the RSO console is shown in Figure 1. If the safety officer had taken destruct action during the time interval from 18 to 25 seconds, impact would have been well away from the flight line. UN CLR55IFIED J O US T1761-R 3D .D ALTE R 1 1 7B E KIN O N TRAC K 1 .0 DE LAY +■ 12 C HEVi 10.7 3 2.2 0.1 4.2 5L0 5HT RG T L ON 170 245 2 HDG VE L RLT a. 14 SKIN O N TRAC K 0.5 DE LAY IF HRF 1 20 SEC. 25 SEC. 18 SEC. 70 G 25 O N 1 .a 1G .5 3 0 1 a.7 4 1 CYBER R 3D D CH E V 15 SEC. M G REEN TRUC K DE LAY O N TRUC K D 5 DE C RY HDG VE L ALT SLO 5HT LFT LO W PRIME C NTRRVE 53 30 SEC. C NTRAVE 53 Figure 1. Joust Impact Trace Showing a M ode-5 Failure Response A s still another example of a M ode-5 failure response, a guided Red Tigress sounding rocket was launched from Pad 20 at C ape C anaveral on 20 A ug 91. W ithin a second or two after clearing the launcher, the rocket made a near 90° right turn, and flew stably in this direction until destroyed by the safety officer at 23.3 seconds. Pieces impacted some two or three miles from the launch pad. This failure might have been classified as a M ode-2 response if destruct action had been taken shortly after launch. 9/10/96 6 RTI 3 . Understanding the Mode-5 Failure Response U nlike failure response M odes 3 and 4, response M ode 5 (and also M ode 2) is not a direct function of time from launch. For M odes 3 and 4, the mean point of impact (M PI) for each debris class is fixed, once the failure time is established. A t each instant there is only one possible location for the M PI for each debris class. On the other hand, die M ode-5 impact­ density function for each debris class consists of a primary part and a secondary superimposed part. The primary impact-density function accounts for impact variability due to the erratic flight of the vehicle. It is used to determine the probability that the mean piece in a debris class resulting from vehicle breakup falls in a given area (say on a building or open field). The secondary density function accounts for debris dispersion due to vehicle breakup and to aerodynamic effects during free fall. It is used to determine the probability that fragments from the class actually hit a building or field. In other words, the primary impact-density function is used to compute the probability that the secondary function is centered in some specified area; the secondary function, which describes the distribution of class pieces about the mean point, is then used to compute the probability that one or more class pieces impacts on the specified population center or area. The primary part of the M ode-5 impact density function, which was presented as Eq. (9.5) in Ref. [1], is reproduced here as Eq. (1): where R is the range from the launch point in miles, ^ is the angle in radians between the uprange direction and a line from the pad through the impact point, R is the impact-range rate in miles per second. A and C are dimensionless shaping constants, and shaping­ constant D is in miles. For a M ode-5 response, there is by definition an earliest time of occurrence Tp (pitch-over time) and a latest time of occurrence TB (burnout, orbital injection, or some other specified termination time). The specific time in this span at which a M ode-5 response manifests itself is of no consequence, although the duration of the span must be considered in assigning a probability of occurrence for a M ode-5 response. G iven that a M ode-5 response has occurred, the probability that the center of the secondary function lies in some region or on some building (population center) is determined by integrating the primary impact-density function for tire class over the region or building. The primary function depends on range (R) and direction (0) from the launch point to the population center, but not directly on time from launch. The primary function does, * As an aid to understanding, the supplement of , designated as 0, is used in plots and tables in this report. 9/10/96 7 RTI however, involve the quantity R which is expressed explicitly as a function of R and only implicitly as a function of time. Values of R from the nominal trajectory are differenced to compute R. The secondary M ode-5 impact-density function is circular normal in form and expressed by the equation f(d) =-^6^ (2) 2nOc where d is the distance from the impact point of the mean piece to the center of the target, and oc is the standard deviation (dispersion) for the debris class. The fact that the center of the secondary impact-density function (or secondary M PI for a debris class) lies on some population center does not necessarily mean that pieces in the class hit the center. The probability that one or more pieces actually hits the pop center is determined by integrating the secondary impact-density function over the center and combining results for all pieces in the class. The dispersions for the secondary function are computed by root-sum­ squaring individual dispersions* arising from the effects of winds, vehicle-breakup velocities, and drag uncertainties for the class. They are computed from the nominal trajectory, and can be explicitly expressed as a function of impact range. Since the pop center can also be hit if the M PI of the secondary density function lies outside the pop center, all possible mutually-exclusive locations of the secondary function that can result in impact on the pop center must be considered. For each mutually-exclusive location, the probability that one or more class pieces impacts on the pop center is calculated, and the results combined to obtain the total hit probability for the class. * These dispersions are a subset of the Mode-4 impact dispersions. The M ode-5 primary impact-density function is modeled so it is independent of how the impact point arrives at a particular location. For example, there are myriad paths that a vehicle can travel to impact at a location two miles crossrange left from the launch pad. Figure 1 shows one such way for a Joust vehicle that failed at 15 seconds, but four seconds later had moved the impact point uprange and crossrange to a position two miles crossrange left from the launch point. A nother way to place the impact point two miles crossrange left is for the vehicle to fly in the wrong direction (north instead of east) from liftoff. A lthough numerous failure mechanisms and vehicle behaviors can lead to a M ode-5 response and impact in a particular area, the exact mechanism and behavior are irrelevant A ll such possibilities are assumed to be accounted for by Eq. (1). Four specific failures that produce M ode-5 responses are easily described: (1) a re-orientation of the guidance platform, (2) insertion of an erroneous spatial target into the guidance system, (3) locking of the engine nozzle in a fixed position near null thus producing a near-constant angular 9/10/96 8 RTI acceleration of the vehicle body and a slow turn of the velocity vector, (4) erroneous accumulation of velocity bite by the guidance system. M any other M ode-5 responses are so convoluted that they defy description or categorization. 3.1 Effects of Mode-5 Shaping Constants The primary part of the M ode-5 impact-density function was presented previously as Eq. (1). A s originally formulated, the function contained three shaping constants. If both numerator and denominator of the equation are divided by the constant C , and B is substituted for D /C , one unnecessary constant disappears so that the function may be expressed as follows: (3) The values chosen for the shaping constants A and B that appear in Eq. (3) influence, but do not change, the basic nature of the M ode-5 impact-density function. For many years values of A = 2.5 and B = 1000 were used in the Eastern Range ship-hit computations, although in more recent risk studies the value of A has been increased to 3.0. This increase resulted from the observation that, in recent years, vehicles that experience M ode-5 failure responses seem less likely than earlier developmental vehicles to deviate significantly from the intended flight line. To see how A and B affect the distribution of M ode-5 impacts, and to further understanding of the function, the results of choosing various values of A and B are provided in A ppendix B. 3.2 Effects of Shaping Constant on D AMP Results A s pointed out in the Introduction, two important types of constant parameters required by D A M P for risk estimations must be determined. They are: (1) probability of a M ode-5 failure response, and (2) values of the M ode-5 shaping constants A and B, currently set at 3.0 and 1000, respectively. A s will be demonstrated later, D A M P results are far more sensitive to changes in A than in B. The following cases illustrate the effects that constant A has on calculated risks. C ase 1: Baseline Risks for A tlas IIA In the baseline risk analysis for A tlas IIA [31, the probability of a M ode-5 failure response was estimated at 12.5% of the total failure probability during the first 120 seconds of flight. Even so, risks resulting from M ode-5 responses accounted for about 90% of the total risks for people inside the impact limit lines (ILL). Table 1 indicates the range of risks inside the ILLs for day launches from Pad A using various estimates of the shaping constant A and a value of B = 1000. 9/10/96 9 RTI Table 1. Effects of M ode-5 Shaping C onstant A on A tlas IIA Risks B = 1,000 Percent of M ode-5 IPs U prange C asualty Expectancy (x 10*) inside ILLs C onstant A ______ M ode 5______ Total for all M odes 2.5 28.6 246 259.9 3.0 20.7 136 149.4 3.5 14.6 58.9 72.7 1 4.0 10.0 30.5 44.3 The results in the third column are directly proportional to the probability that a M ode- 5 failure occurs. For the A tlas IIA analysis, a value of 1/200 = 0.005 was assumed. C ase 2: Risk C ontours for A tlas H A S D efinitions of Flight Hazard Area and Flight Caution Area may be based on the risk contours for inner-ear injury. C onstant A can have a significant effect on the location of the 10* contour, as illustrated in Figure 2 and Figure 3 for the A tlas IIA S. For these figures, the M ode-5 absolute probability of occurrence was 0.005, constant A was 3.0 and 3.5, and constant B was 1000. 9/10/96 10 RTI Figure 2. A tlas H A S Risk C ontours for Inner-Ear Injury with A = 3.0 9/10/96 11 RTI Figure 3. A tlas H A S Risk C ontours for Inner-Ear Injury with A = 3.5 9/10/96 12 RTI 4. Methodology for Assessing Failure Probabilities A primary purpose of this study is to develop estimates of the relative probabilities of occurrence of a M ode-5 failure response for A tlas, D elta, Titan, and as a by-product, for other launch vehicles as well. Natural fallouts of this effort are the relative probabilities of occurrence of other failure-response modes used in program D A M P as well as overall vehicle failure probabilities. There are at least two approaches commonly used in estimating launch-vehicle failure probabilities: (1) a so-called parts-analysis or engineering approach, involving an engineering assessment of the reliability of various parts and components comprising each missile subsystem, and the effects of a part, component or subsystem failure; and (2) an empirical statistical approach based on actual launch results. There are serious problems with both approaches. 4.1 The Parts-Analysis Approach A description of this approach, its difficulties and shortcomings, are discussed in some detail in a draft report by Booz • A llen & H amilton, Inc.141 prepared in 1992 for the A ir Force Space C ommand. Since we cannot improve on the ideas and words expressed by Booz* A llen, we quote the following from that report "The engineering approach for calculation of launch vehicle success rates is based on measurement/estimation of piece-part reliabilities and their combination into reliability block models of the launch system. These block models ... include consideration of the criticality of individual components, the presence (or absence) of redundant capabilities, the likelihood that one component failure might cause a failure in another component, as well as other needed data. By combining the individual piece-part reliabilities in this model, the engineering approach produces an overall reliability estimate for the launch system. "The engineering approach has several significant limitations that tend to reduce confidence in its results. First, the approach assumes that the interrelationships among and between sub-systems are understood sufficiently to enable development of a reliability block diagram. This assumption is highly questionable in complex systems, such as space launch vehicles, whose operational histories include many anecdotes regarding unexpected relationships between 'independent' sub-systems. "The second drawback of the engineering approach is that it assesses the reliability of the system in a perfectly assembled condition. A s a result, it assesses reliability without regard to manufacturing, processing, or operations variations and errors." Effects typically overlooked or ignored include: a. Improper installation of components b. Erroneous computer programs 9/10/96 13 RTI c. Insertion of improper computer programs d. Support-personnel fatigue A third limitation of the parts-analysis approach discussed in Ref. [4] deals with the subjectivity and invalid assumptions often used to'estimate piece/component reliabilities. H ere Booz# A llen quotes from a report'51 by the Office of Technology A ssessment, and we do likewise: "The design reliability of proposed vehicles is generally estimated using: D ata from laboratory tests of vehicle systems (e.g., engines and avionics) and components that have already been built; Engineer’s judgments about the reliability achievable in systems and components that have not been built; A nalyses of whether a failure in one system or component would cause other systems and components, or the vehicle to fail; and A ssumptions (often tacit) that: the laboratory conditions under which systems were tested precisely duplicate the conditions under which the systems will operate, the conditions under which the system will operate are those under which they were designed to operate, the engineer's judgments about reliability are correct, and the failure analyses considered all circumstances and details that influence reliability; Such engineering estimates of design reliability are incomplete and subjective...". Effects influencing reliability that the analyst may fail to consider include: a. Lightning strikes b. A ging effects, particularly for solid propellants c. C orrosion d. Insufficient heat or cold insulation for critical components e. Icing f. Erroneous antennae patterns or instrumentation Booz* A llen concludes as follows: "Finally, due to its nature, the engineering approach can not account for undetected design flaws. (If these flaws were detected, and could be modeled, 9/10/96 14 RTI they would be corrected.) H owever, experience has shown that design flaws do cause failures in operational launch systems, and will likely do so in the future." The major objection to the parts-analysis approach, hinted at above but not actually expressed, is that all such approaches involve either explicitly or implicitly a so-called K - factor. The K -factor is included in the reliability calculations in an attempt to compensate for the fact that the environment in which a part or system is tested is not the same as the flight environment. Since the K -factor is surely not the same for all components and systems, multiple values must be assumed and the entire process becomes highly subjective. In view of the objections and limitations just presented, in this report the parts-analysis approach is not considered in assessing vehicle reliability or in estimating the relative probabilities of occurrence of the various failure-response modes. 4.2 The Empirical Approach A seemingly more objective way to evaluate vehicle reliability (or conversely, vehicle failure probabilities) is by examining the actual performance of flight-tested vehicles. In support of this approach, the following is quoted from the Office of Technology A ssessment151 report previously referenced: "The only completely objective method of estimating a vehicle's probability of failure is by statistical analysis of number of failures observed in identical vehicles under conditions representative of those under which future launches will be attempted." A lthough we agree with the Office of Technology A ssessment statement, the obvious difficulty with this approach is that no such sample of identical vehicles exists or is ever likely to exist. In their report141 previously referenced, Booz* A llen makes the same point in different words by stating that "the empirical approach has one significant drawback in that it can not project the effects of changes in the launch systems". The effects of such changes can only be assessed objectively by further flight testing. The difficulty in projecting success rates (or failure rates) from past tests to future tests is clearly recognized. Nevertheless, RTI has relied exclusively on this method to estimate the relative probabilities of occurrence for the various failure-response modes. Even so, total objectivity cannot be claimed since, as will be seen later, the answers depend to a large extent on how the performance data are filtered, and how big a risk one wants to take that the true failure probability is underestimated. 9/10/96 15 RTI 5. C omputation of Failure Probabilities The test results for A tlas, D elta, and Titan in the tables of A ppendix D have been used for three primary purposes: (1) To predict or estimate the Overall probability that each vehicle will fail during the various phases of flight (see Table 39, A ppendix D , for flight-phase definitions). (2) To establish the relative and overall probabilities for Response M odes 1 through 5. (3) To establish the relative frequency of tumble for Response M odes 3 and 4. 5.1 Overall Failure Probability To predict failure probabilities for A tlas, D elta, and Titan, the test results in A ppendix D for representative configurations (i.e., "1" in last column) have been filtered using three different weighting techniques described in A ppendix C : (1) Equal weighting (2) Index-count weighting (3) Exponential weighting In computing filtered or weighted failure probabilities, a test is assigned a score of one to indicate the occurrence of a failure or some anomalous behavior, and a score of zero if no failure occurred. A dmittedly, there may be disagreements about the classification of a few flights, since the launch agency may consider as successful or partially successful some flights that are shown as failures in A ppendix D . To avoid such disagreements, it is better to think of some non-normal events, particularly those occurring late in flight, as anomalies rather than failures. The flight phases, as shown in column 2 of Table 2 and defined in A ppendix D .1.3, are inclusive; e.g., flight phase "0 - 3" includes phases 0,1,1.5,2,2.5, and 3. A n 'NA ' in the response-mode column in the tables of A ppendix D indicates that some failure or anomalous behavior has had an effect on the final orbit or impact point without producing additional risks to people on the ground or necessarily failing the mission. In the failure-probability calculations of Table 2 and Table 3, an 'NA ' has been- considered as a success for all flight phases except "0 - 5", irrespective of the phase in which the failure or anomalous behavior took place. Only in flight phase "0 - 5" is an ZNA ' response considered a failure. The filtered results for representative configurations (defined in A ppendix D .1.4) are given in Table 2 for six flight phases. For flights with multiple entries in the Response-M ode and Flight-Phase columns (e.g., see A ppendix D .2.1, No. 257), the first listed value was used in the filtering process. 9/10/96 16 RTI Table 2. Predicted Failure Probabilities for Representative C onfigurations Vehicle Flight Phase Filter Technique Sample Failures /Total Equal W eight Index C ount Expon. F = 0.99 Expon. F = 0.98 Expon F = 0.97 A tlas 0 0 0 0 0 0 0/7 0-1 0.0256 0.0253 0.0245 0.0219 0.0186 4/156 0-2 0.0449 0.0385 0.0387 0.0313 0.0243 7/156 0-3 0.0769 0.0715 0.0714 0.0643 0.0568 12/156 0-4 0.0833 0.0811 0.0801 0.0740 0.0663 13/156 0-5* 0.1090 0.1100 0.1078 0.1019 0.0929 17/156 D elta 0 0 0 0 0 0 0/125 0-1 0.0160 0.0126 0.0134 0.0104 0.0075 2/125 0-2 0.0160 0.0126 0.0134 0.0104 0.0075 2/125 0-3 0.0160 0.0126 0.0134 0.0104 0.0075 2/125 0-4 0.0160 0.0126 0.0134 0.0104 0.0075 2/125 0-5* 0.0640 0.0447 0.0535 0.0469 0.0442 8/125 Titan 0 0.0306 0.0210 0.0225 0.0292 0.0352 3/98 0-1 0.0234 0.0305 0.0314 0.0403 0.0470 4/171 0-2 • 0.0409 0.0496 0.0514 0.0642 0.0750 7/171 0-3 0.0526 0.0581 0.0597 0.0689 0.0773 9/171 0-4 0.0526 0.0581 0.0597 0.0689 0.0773 9/171 0-5* 0.1111 0.1167 0.1188 0.1284 0.1358 19/171 * Includes response mode 'NA ' It is apparent from the data in Table 2 that estimates of future vehicle reliability depend on the filtering (i.e., weighting) technique applied. Since there are many ways to perform the filtering, all generally producing slightly different results, the choice of method to use in deriving empirical failure probabilities cannot be totally objective. Subjective decisions must also be made about which past configurations to consider as representative of future vehicles, which flight tests to include in the sample, how to weight the individual flights, and, in unusual cases, whether to consider a flight a success or a failure, and to which flight phase to attribute a failure. Except for data weighting (i.e., choice of filter), these decisions were made for A tlas, D elta, and Titan before computing the failure probabilities shown in Table 2. For A tlas and D elta, it can be seen from Table 2 that the predicted failure probabilities computed with the exponential filter decrease as the value of F decreases. Since a decreasing F means more emphasis on recent data and less emphasis on the old, the launch reliability for these vehicles is apparently improving. The reverse seems to be true for Titan, suggesting either that Titan reliability is not improving or, possibly, that improvements that have been or are being made to the vehicle are not yet fully reflected in the test results. For A tlas and D elta, the computed failure probabilities based on equal weighting are higher than for all other filters, and the predicted failure 9/10/96 17 RTI probabilities using index-count filtering are larger than those for exponential filtering. For Titan, the results are mixed, further suggesting that Titan reliability has not improved in recent years. For comparison purposes, the same filtering techniques have been applied to all flight tests shown in the tables of A ppendix D , regardless of configuration. The results are presented in Table 3. * Includes response mode 'NA ' Table 3.Predicted 1failure Probabilities for A ll C onfigurations___________ Filter Technicue Sample Flight Equal Index Expon. Expon. Expon. Failures Vehicle Phase W eight C ount F = 0.99 F = 0.98 F = 0.97 /Total A tlas 0 0 0 0 0 0 0/7 0-1 0.1053 0.0641 0.0422 0.0273 0.0190 56/532 0-2 0.1711 0.0990 0.0555 0.0311 0.0204 91/532 0-3 0.2086 0.1261 0.0802 0.0559 0.0455 111/532 0-4 0.2143 0.1330 0.0873 0.0627 0.0511 114/532 0-5* 0.2575 0.1671 0.1150 0.0866 0.0725 137/532 D elta 0 0 0 0 0 0 0/196 0-1 0.0172 0.0164 0.0148 0.0110 0.0077 4/232 0-2 0.0259 0.0232 0.0201 0.0133 0.0085 6/232 0-3 0.0431 0.0279 0.0263 0.0150 0.0089 10/232 0-4 0.0431 0.0279 0.0263 0.0150 0.0089 10/232 0-5* 0.1078 0.0766 0.0740 0.0536 0.0459 25/232 Titan 0 0.0306 0.0137 0.0187 0.0281 0.0349 3/98 1 0-1 0.0534 0.0319 0.0351 0.0399 0.0467 18/337 0-2 0.1424 0.0771 0.0719 0.0662 0.0750 48/337 0-3 0.1632 0.0924 0.0830 0.0711 0.0770 55/337 0-4 0.1662 0.0942 0.0840 0.0712 0.0771 56/337 0-5* 0.1958 0.1369 0.1326 0.1277 0.1346 _66/337_ A comparison of Table 2 and Table 3 shows that in most cases, but not all, exponential filtering produces failure probabilities for the representative configuration samples that are smaller than the corresponding probabilities for the all-configuration samples. The fact that most differences between corresponding samples are relatively small attests to the effectiveness of the exponential filter in down-weighting early launch failures. This is not the case for equal weighting of tests, where the predicted failure probabilities based on all configurations are up to 3.6 times as large. W ith respect to the weighting of missile and space-vehicle performance data, RTI favors an exponential filter over either the equal-weight or index-count filters. W eighting percentages for the three filters are given in Table 4 for sample sizes of 4 to 1,000. Except for small samples, the percentages produced by equal weighting place too much emphasis on old data, thus failing to account for the learning process and 9/10/96 18 RTI hardware improvements that have taken place through the years. For samples approaching 100 or so, it seriously over-weights the old data and under-weights the more recent events. A lthough equal weighting does not seem suitable for this application, it could be appropriate in other large-sample situations, for example, predicting the failure probability of devices that are all manufactured at the same time by the same process, and tested to the same standards. * F = 0.98 for exponential filter + "Last" refers to the most recent data point ?able 4. C omparison of W eighting Percentages____________________ Sample Last + Last 5 Last 10 Last 25 Last 50 Last Size Filter * Point Points Points Points Points H alf 4 Expon. 25.8 • . 51.0 Index 40.0 * — a 70.0 Equal 25.0 • — - 50.0 10 Expon. 10.9 52.5 100.0 - - 52.5 Index 18.2 72.7 100.0 72.5 Equal 10.0 50.0 100.0 - - 50.0 20 Expon. 6.0 28.9 55.0 - 55.0 Index 9.5 42.9 73.8 • 73.8 Equal 5.0 25.0 50.0 50.0 100 Expon. 2.3 11.1 21.1 45.7 73.3 73.3 Index 2.0 9.7 18.9 43.6 74.8 74.8 Equal 1.0 5.0 10.0 25.0 50.0 50.0 200 Expon. 2.0 9.8 18.6 40.4 64.7 88.3 Index 1.0 4.9 9.7 23.4 43.7 74.9 Equal 0.5 2.5 5.0 12.5 25.0 50.0 500 Expon. 2.0 9.6 18.3 39.7 63.6 99.4 Index 0.4 2.0 4.0 9.7 19.0 75.0 Equal 0.2 1.0 2.0 5.0 10.0 50.0 1000 Expon. 2.0 9.6 18.3 39.7 63.6 99.996 Index 0.1 1.0 2.0 4.9 9.7 75.0 Equal 0.1 0.5 1.0 2.5 5.0 50.0 The index-count filter has serious deficiencies when applied to either small or large samples of missiles and space vehicles. For small samples, too much emphasis is placed on recent data. For a sample of four, 40% of the total weight is given to the last test, and 70% to the last two tests. For a sample of ten, 18.2% of the total weight is given to the last test and 72.7% to the last five tests. The reliability improvement rate implied by these weightings seems too optimistic unless there were serious design flaws in the early configurations that were discovered and corrected. Since many types of failures surely exist that occur only once in 50 or once in 100 or more launches, the tenth launch may be no better than the first for predicting the probability of occurrence of such failures. For large samples, the index-count filter under-weights current data 9/10/96 19 RTI more and more as the sample size increases. For samples of 200, 500, and 1000, the weighting of the last 50 tests are, in each case, 43.7% , 19.0% , and 9.7% of the total weight. For samples of 100 or more, no matter how large, the index-count filter assigns 25% of the data weight to the oldest half of the data sample - too much in RTFs opinion. For missiles and space vehicles, the data weightings imposed by the exponential filter (F = 0.98) appear reasonable. For small samples less than 20 or so, there is little difference between equal and exponential weightings. For sample sizes near 80, the index-count and exponential filters produce similar results. For sample sizes of 200 and more, the weights assigned to the most recent 5,10, 25, and 50 tests are essentially constant, showing the fading-memory nature of the exponential filter. The denominator of the exponential-filter equation [Eq. (18), A ppendix C ] is a geometric series that asymptotically approaches a limit of [1/(1 -F)] as n approaches infinity. For F = 0.98, that limit is 50. Thus, the last data point, which is always given a weight of one, can never be weighted less than 2% of the total, no matter how large the sample. For samples of 200 and 300, the oldest half of the data receives only 11.7% and 5% of the total weight. For samples of 500 and larger, the oldest half of the data sample is essentially omitted altogether. The exponential filter is clearly a fading-memory filter, as it should be for space-vehicle performance data. H aving decided upon the exponential filter as the best method for weighting missile and space-vehicle performance data, a filter constant F must be chosen. To see how data weighting varies with filter-factor value, weighting percentages for various samples were computed for representative configurations of A tlas, D elta, and Titan using values of F from 0.96 to 0.995. The results are shown in Table 5. 9/10/96 20 RTI * Last half + 1 if sample size is odd ________________Table 5. Filter Factor Influence on W eigiting Percentages Vehicle (sample) Filter C ons't Last Point Last 10 Points Last 50 Points Last H alf* Last 100 Points Pt. Ratio last: first , A tlas 0.96 4.01 33.6 87.2 96.0 98.5 560 (156) 0.97 3.03 26.5 78.9 91.5 96.1 112 0.98 2.09 19.1 66.4 82.9 90.6 22.9 0.99 1.26 12.1 49.9 68.7 80.1 4.7 0.995 0.92 9.0 40.9 59.7 72.7 2.2 D elta 0.96 4.02 33.5 87.5 92.9 98.9 158 (125) 0.97 3.07 26.9 80.0 87.3 97.4 43.7 0.98 2.17 19.9 69.1 78.3 94.3 12.2 0.99 1.40 13.4 55.2 65.6 88.6 3.5 0.995 1.07 10.5 47.6 58.2 84.7 1.9 Titan 0.96 4.00 33.5 87.1 97.1 98.4 1030 (171) 0.97 3.02 26.4 78.6 93.2 95.8 177 0.98 2.07 18.9 65.7 85.1 89.6 31.0 0.99 1.22 11.7 48.1 70.5 77.2 5.5 0.995 0.87 8.5 38.5 60.8 68.5 2.3 A lthough the choice of a filter constant cannot be completely objective, use of a value less than 0.97 or greater than 0.99 produces undesirable weightings. For F = 0.96, for example, the most recent test result for Titan is weighted 1030 times that for the oldest test; the last 50 data points receive 87.1% of the total weighting, leaving only 12.9% for the first 121 flights; the last 100 flights receive 98.4% of the total weighting thus, in effect, omitting the oldest 71 flights from the solution. A t the high end of the F spectrum, a value of 0.995 fails to down-weight the old test results sufficiently. U sing A tlas as an example, the most recent data point (1/31/96) is weighted only 2.2 times that of the oldest data point (8/14/64). The oldest half of the data, stretching from 8/14/64 to 3/06/73, receives 40% of the total weight, and the earliest 56 launches, comprising 36% of the data, receive 27% (100 - 73) of the total weight. This is not too different from equal weighting of tests, a procedure that fails to acknowledge the improvements in A tlas reliability that have taken place over a period of 32 years. In choosing a value of F, an attempt is made to strike a suitable balance between two contrary objectives: (1) to down-weight substantially those failures for which the probability of occurrence has been greatly reduced through redesign and replacement of components, improved test procedures, and the like; 9/10/96 21 RTI (2) to down-weight only slightly, or not at all, those failures that are random in nature, that can still occur in replacement components, or that occur only once in 100 or several hundred launches in components that have not yet failed. No matter what technique is employed, filtering is at best a compromise. The perfect filter would somehow down-weight to some extent or entirely those failures that have been "fixed" or made less likely, without down-weighting those random failures with unknown causes. The filters considered in this study have no such capabilities; they produce a result based solely on the launch sequence, and where in the sequence failures have occurred. In predicting vehicle failure probabilities from empirical data, large representative samples are essential for a good estimate, and the more reliable the vehicle, the greater the need for a large sample. For example, if some characteristic exists in exactly 1% of a population, the probability is 0.37 that it will not appear in a random sample of 100, and 0.61 that it will not appear if the sample size is 50. If the characteristic exists in 2% of the population, it fails to'appear about 36% of the time in a random sample of 50. For reasons presented above, the data samples for A tlas, D elta, and Titan have been made as large as possible consistent with the notion of representative configurations, as set forth in Ref. [4]. In RTFs judgment, the value of F that best weights the performance data is 0.98, although a value anywhere in the interval 0.97 to 0.99 cannot be ruled out. For consistency in data weighting, the same values of F have been used for all vehicle programs. The differences in predicted failure probability that result from these three F's are illustrated in Figure 4 for A tlas. The plots show the inverse relationship between filter volatility and the value of F. For F = 0.97 vis-J-vis larger values, it can be seen that the filtered failure probability jumps higher with each failure and drops at a faster rate with each successful launch that follows. 9/10/96 22 RH Figure 4. Filter Factor Results for Representative C onfigurations of A tlas In summary, it must be recognized that there is no "correct" value for F, and that it is even difficult to argue generally that one value of F is better than another. In RTFs view, values of F below 0.97 place too much emphasis on a relatively small sample of recent launches. Values above 0.99 extend the sample so far back in time that too little emphasis is placed on improvements in design, materials, and operational procedures. In any event, the value chosen for F is crucial in arriving at a predicted failure probability. For the more conservative, a value of 0.99 can be chosen; the optimistic might chose 0.97. Since most risk-analysis studies that RTI makes are concerned with the launch area, failure probabilities beyond flight-phase 2 are of minor interest. The overall failure probabilities shown in Table 6 have, with one exception, been extracted from Table 2 for F = 0.98. W here a best estimate is called for, RTI plans to use these probabilities in future launch-area risk analyses for the 45SW /SE unless directed otherwise, or until additions to the data samples in A ppendix D justify changes. 9/10/96 23 RTI Table ^Failure Probabilities for A tlas, D elta, and Titan Predicted Failure Probability * Vehicle Flight Phase 0-1 Flight Phase A tlas 0.022 0.031 D elta 0.010 0.013 Titan 0.040 0.064 * Exponential filter with F = 0.98 For D elta, the predicted failure probabilities shown in Table 2 for flight-phases 0-1 and 0-2 are the same, since no second-stage failure has occurred in the 125 flights included in the representative sample. Obviously, this does not mean that the probability of a D elta second-stage failure is zero. A s stated earlier, the choice of F is a judgment matter with the most reasonable range for F considered to be 0.97 < F < 0.99. To show a difference in failure probabilities between D elta flight phases, a value of F = 0.98 has been used for flight phases 0-1, and 0.99 for flight phases 0-2. It is an interesting coincidence that the same value of 0.013 is obtained using F = 0.98 and all D elta configurations (see Table 3). A nother way to estimate the D elta second-stage failure probability is to calculate an upper confidence limit at some suitable level for an event that has occurred zero times in 125 trials. A t the 80% confidence level, the reliability is at least 0.987, so the failure probability during second-stage bum (flight phases 1.5 - 2) is no bigger than 0.013. 5.2 Relative and Absolute Probabilities for Response Modes For A tlas, D elta, and Titan vehicles, failure-response M odes 1, 2, and 3 are much less likely to occur than M odes 4 and 5. Since the probabilities of occurrence for the less- likely modes may be only one in a thousand or less, such responses may not have occurred at all in the flight tests of representative configurations. In fact, in the combined samples for A tlas, D elta, and Titan, only 16 failures have occurred during flights phases 0-2. None of the 16 resulted in response-modes 1, 2, or 3. Because of the small number of failures in the representative configuration samples, the relative probabilities of occurrence for M odes 1 through 5 have been estimated using results from all vehicle configurations and launches shown in A ppendix D . The rationale for this approach is that, except for obvious problems that have been corrected, other changes made through the years to improve vehicle reliability have reduced the probabilities of occurrence of all response modes more or less proportionally. The greater significance of more recent vehicle modifications and test resulte is accounted for by using an exponential filter to estimate overall failure probabilities. Thus, if M ode-1 failures occurred more frequently in the distant past than in recent years, the weighting process reduces the significance of the earlier M ode-1 responses in the relative probability-of-occurrence calculations. A s tabulated from A ppendix D , the number (count) of failures by response mode and flight phase for A tlas, D elta, Titan, and Eastern-Range Thor launches are given in Table 7 through Table 10. Thor launches 9/10/96 24 RTI from the W estern Range were not included since available performance records were incomplete. The results for the four vehicles are combined in Table 11. Table 12 gives last-occurrence dates by response mode for each launch vehicle. Table 7. Number of A tlas Failures - A U C onfigurations (532 Flights) Flight Fai:ure-Res]ponseM ode 3&4 Phase 1 2 4 =2=W Tumble 0 0 0 0 0 0 0 0 0-1 7 1 2 38 8 4 11 0-2 7 1 2 66 15 13 19 0-3 7 1 2 86 15 18 25 0-4 7 1 2 89 15 21 27 0-5 7 1 2 89 15 23 27 Table 8. Number of D elta Failures - A ll C onfigurations (232 Flights) Flight Phase Failure-Response M ode 3 & 4 Tumble1 2 3 4 5 'NA ' 0 0 0 0 0 0 0 0 0-1 0 0 0 2 2 5 0 0-2 0 0 0 4 2 10 1 0-3 0 0 0 7 3 12 1 0-4 0 0 0 7 3 13 1 0-5 0 0 0 7 — 3 15 1 Table 9. Number of Titan Failures; - A ll C onfigurations (337 Flights) Flight Faiure-Res]ponse M ode 3&4 Phase 1 2 3 4 5 'NA ' Tumble 0 0 0 0 3 0 0 1 0-1 2 2 0 13 1 0 5 0-2 2 2 0 39 5 3 10 0-3 2 2 0 46 5 5 11 0-4 2 2 0 47 5 7 11 0-5 2 2 0 47 5 10 11 Table 10. Number of Eastern-Range Thor Failures (85 Flights) Flight Phase Failure-Response M ode 3&4 Tumble1 2 3 4 5 'NA ' 0 0 0 0 0 0 0 0 0-1 4 1 1 15 4 1 3 0-2 4 1 1 20 5 3 3 0-3 4 1 1 22 5 3 3 0-4 4 1 1 22 5 4 3 0-5 4 1 1 22 5 5 3 9/10/96 25 RTI Table 12. D ate of M ost Recent Failure Table 11. Number of Failures for A ll Vehicles (1186 Flights) Flight Faiure-Res]ponse M ode 3&4 Phase 1 =2= 3 4 'NA ' Tumble 0 0 0 0 3 0 0 1 0-1 13 4 3 68 15 11 19 0-2 13 4 3 129 27 29 33 0-3 13 4 3 161 28 38 40 0-4 13 4 3 165 28 45 42 0-5 13 4 3 165 28 53 42 * Last Thor launch was 02/23/65 Response Vehicle M ode A tlas D elta Titan Thor* 1 03/02/65 none 12/12/59 04/19/58 2 12/18/81 none 05/01/63 12/30/58 3 04/25/61 none none 07/21/59 4 08/22/92 05/03/86 10/05/93 03/24//64 5 12/08/80 08/27/69 11/30/65 01/24/62 For the reasons advanced previously, an exponential filter has been used to estimate relative probabilities of occurrence for M odes 1 through 5 and the fraction of M ode-3 and M ode-4 failures that tumble while the vehicle is thrusting. The percentage weightings for various data samples are shown in Table 13 for values of F from 0.980 to 0.999. Because of the large size of the composite sample (1186), the filter-control constant of 0.98 used previously to estimate absolute failure probabilities for individual vehicles does not seem suitable for estimating relative probabilities for the individual response modes. U se of 0.98 would effectively place 98.2% of the total weight on the most recent 200 tests thus, in effect, eliminating the earliest 986 tests from the solution. These are the very tests needed to provide an adequate sample of failures from which to estimate relative frequencies of occurrence of the individual response modes. 9/10/96 26 RTI Table 13. Percentage W eighting for Sample of 1186 Launches Filter C onstant Last Point Last 100 Points Last 200 Points Last 300 Points Last 500 Points Point Ratio Last:First 0.999 0.14 13.7 26.1 37.3 56.7 3.3 0.996 0.40 33.3 55.6 70.6 87.3 1.2 x 102 0.995 0.50 39.5 63.5 78.0 92.1 3.8 x 102 0.994 0.60 45.3 70.0 83.6 95.1 1.3 x 103 0.993 0.70 50.5 75.5 87.9 97.0 4.2 x 103 0.992 0.80 55.2 79.9 91.0 98.2 1.4x10* 0.991 0.90 59.5 83.6 93.4 98.9 4.5 x 104 0.990 1.00 63.4 86.6 95.1 99.3 1.5 x 105 0.980 2.00 86.7 98.2 99.8 99.996 3.9x10” The value of F = 0.999 is considered inappropriate because, as seen in Table 13, the weighting factor applied to the most recent datum is only 3.3 times that applied to the oldest test result from 39 years ago. The most recent 200 and 300 points in the sample comprising 16.8% and 25.2% of the data receive only 26.1% and 37.3% of the total weight. This is not too different from equal weighting of data, which is appropriate only if the relative frequency of occurrence of each response mode has not changed significantly through the years. On the other hand, use of F = 0.99 effectively throws out the oldest 600 to 700 launches that are sorely needed for an adequate sample size. The results of the filtering process are given in Table 14 for failures during flight phases 0-2. Table 14. Response-M ode Occurrence Percentages .. Filter Response M ode Factor 1 2 3 4 5 0.999 7.39 2.27 1.70 73.30 15.34 0.996 2.24 4.35 0.37 80.37 12.67 0.995 1.32 4.92 0.19 82.59 10.98 0.994 0.73 5.26 0.09 84.57 9.35 0.993 0.39 5.37 0.04 86.25 7.95 0.992 0.20 5.31 0.02 87.68 6.78 0.991 0.11 5.13 0.01 88.92 5.84 0.990 0.05 4.87 0.00 90.02 5.06 0.980 0.00 1.86 0.00 96.81 1.33 The results in Table 14 show that the percentages of occurrence for response-modes 2 and 4 are relatively insensitive to filter-factor values, while the percentages for M odes 1, 3, and 5 decrease as filter memory (filter factor) decreases. This suggests that occurrences of M odes 1, 3, and 5 have been decreasing over the years, while M odes 2 and 4 occurrences have not changed much. A lthough it cannot be argued convincingly 9/10/96 27 RTI that 0.993 is superior to 0.992 or 0.994, or even values outside this interval, a value of 0.993 was chosen. This section has thus far described a rationale for selecting a filtering process and filter constant to estimate percentages of occurrence of failure-response modes for A tlas, D elta, and Titan launch vehicles. These are mature launch systems with improved reliability as a result of years of experience and corrections of problems. A lthough the designs of new launch vehicles may be based to some extent on mature systems, new systems are expected to fail at a higher rate. For vehicles with liquid-propellant stages burning at liftoff, the percentages of occurrence of the various response modes are more likely to be similar to the earlier versions of A tlas, D elta, and Titan than to current vehicles. For lack of any other data, for such new liquid-propellant systems the relative percentages for the five failure-response modes have been calculated using the total combined sample of A tlas, D elta, Titan, and Thor with a filter constant of 0.999 (almost equal weighting). For new solid-propellant vehicles, use of F = 0.999 results in a M ode-1 percentage that seems much too high. A ll of the 13 M ode-1 failures in the composite sample (Table 11) involved liquid-propellant vehicles, whereas none of the A tlas, D elta, or Titan configurations with solid-propellant boosters have experienced a M ode-1 response. On the other hand, use of F = 0.993 that is applied for mature launch systems seems to reduce the probability of a M ode-5 response too much, since a Red Tigress vehicle and a Joust vehicle launched at the C ape in 1991 both experienced M ode-5 failure responses (see Section 2). A s a compromise between new and mature liquid-propellant vehicles, a value of F = 0.996 has been assumed for new solid-propellant vehicles. The percentages shown in Table 15 for flight phases 0-2 have been obtained from Table 14. Similar information for flight phases 0-1 are given in Table 16. In future risk studies for the 45 SW /SE, RTI plans to use these relative percentages for mature and new systems. Table 15. Recommended Response-M ode Percentages for H ight Phases 0-2 Response M ode M ature Launch Systems (F = 0.993) New Solid Systems (F = 0.996) New Liquid Systems (F = 0.999) 1 0.4 2.2 7.4 2 5.4 4.3 2.3 3 0.1 0.4 1.7 4 86.2 80.4 73.3 5 7.9 12.7 15.3 9/10/96 28 RTI Table 16. Recommended Response-M ode Percentages for Flight Phases 0 -1 Response M ode M ature Launch Systems (F = 0.993) New Solid Systems (F = 0.996) New Liquid Systems (F = 0.999) 1 0.5 3.4 10.7 2 7.4 6.6 4.3 3 0.1 0.6 2.4 4 81.9 74.5 67.0 5 __________ 10.1________ 14.9 15.6 A bsolute probabilities of occurrence for response M odes 1 through 5 can be obtained by multiplying the absolute failure probabilities for flight phases 0-1 and 0-2 (Table 6) by the relative failure probabilities in Table 15 and Table 16. The results are shown in Table 17. Probabilities are listed to six decimal places to show differences, not because all figures are actually significant. To obtain these results, more precise values for relative probabilities of occurrence were used than shown in Table 15 and Table 16. Table 17. A bsolute Failure Probabilities for Response M odes 1-5 Vehicle: A tlas D elta Titan Flight Phase: 0-1 (0-170 sec) 0-2 (0-280 sec) 0-1 (0-270 sec) 0-2 (0-630 sec) 0-1 (0-300 sec) 0-2 (0-540 sec) M ode 1 0.000119 0.000121 0.000054 0.000051 0.000216 0.000250 M ode 2 0.001637 0.001665 0.000744 0.000698 0.002976 0.003437 M ode 3 0.000011 0.000012 0.000005 0.000005 0.000020 0.000026 M ode 4 0.018007 0.026738 0.008185 0.011212 0.032740 0.055200 M ode 5 0.002226 0.002465 0.001012 0.001034 0.004048 0.005088 Total 0,022 0.031 0.010 0.013 0.040 0.064 For each vehicle, the absolute probabilities for M odes 1,2, and 3 differ slightly for flight phases 0-1 and 0-2. This difference is due to the unequal data weighting produced by the exponential filter. If equal data weighting had been applied, the absolute probabilities for these modes would have been identical as expected, since M odes 1, 2, and 3 cannot occur beyond flight phase 1. D ifferences in absolute probabilities for M odes 4 and 5 for flight phases 0-1 and 0-2 can also be seen in the table. A part of this difference may result from unequal data weighting, but primarily it is due to the obvious fact that fewer M ode 4 and 5 failures have occurred during flight phase 0-1 than during the longer span of flight phase 0-2. 9/10/96 29 RTI 5.3 Relative Probability of Tumble for Response-Modes 3 and 4 Exponential filters with values of F from 0.98 to 0.999 have been used to estimate the percentage of M ode-3 and M ode-4 responses that terminate with a thrusting tumble. Results are given in Table 18 for flight phases 0-2 and 0-5. For launch-area risk calculations, only flight phases 0-2 are of interest. The data sample was a chronological composite of all A tlas, D elta, Titan, and Thor tests and configurations shown in A ppendix D . To several decimal places at least, the values in the table are determined entirely from M ode-4 responses, since the last vehicle to experience a M ode-3 response (4/25/61) is weighted out of the solution; The results in Table 18 are based on a total sample size of 1,186 flight tests. Table 18. Percenof Response M odes 3 and 4 That Tumble Filter Factor Flight Phases 0-2 Flight Phases 0-5 0.999 25.0 25.0 0.996 26.3 27.0 0.993 27.3 28.6 0.990 28.3 30.1 0.980 31.3 34.8 Through flight phase 2, there were 33 tumbles out of a total of 132 M ode-3 and M ode-4 responses. Through flight phase 5, there were 42 tumbles out of 168 M ode-3 and M ode-4 responses. A s seen from Table 13, the smaller the filter factor, the greater the weight placed on recent test data. In view of this, it is apparent from Table 18 that the percentage of M ode-4 responses that end with a thrusting tumble has been increasing gradually. The same conclusion is reached for flight phases 0-2 and 0-5. In recognition of this gradual increase, in future studies RTI will assume that approximately one-third of M ode-3 and M ode-4 failure responses end with a thrusting tumble. 9/10/96 30 RTI 6. Shaping C onstants Through Simulation Since adequate test data are not available to establish the M ode-5 shaping constants empirically, other methods are needed for this purpose. It will be recalled that, after vehicle pitchover, any malfunction with the potential to cause a substantial deviation from the intended flight line is, by definition, a M ode-5 failure response. The malfunction need not actually cause a large deviation to be classified as a M ode-5 response. One such class of failures leading to a M ode-5 response has been termed a random-attitude failure. Such responses can result from guidance and control failures that lead to erroneous orientation of the guidance platform or an erroneous spatial target. A nother class of failures that can cause sustained deviation away from the flight line is the slow turn, where the engine nozzle, in effect, locks in some fixed position, generally but not necessarily near null. Both types of malfunctions have been investigated in an attempt to estimate numerical values for M ode-5 shaping constants A and B. Basically, the idea is to (1) run a large sample of random-attitude and slow-tum failures, (2) calculate the percentages of impacts in five-degree sectors from 0° to 180°, (3) compare these percentages with those obtained from the M ode-5 impact density function when specific values are assigned to A and B, and (4) assign values to A and B until the best possible fit is obtained between the simulated-turn impacts and the theoretical M ode-5 impacts. 6 .1 Malfunction Turn Simulations 6 .1.1 Random-Attitude Failures A guidance and control failure leading to a fixed erroneous direction of thrust is termed a random-attitude failure. Such failures represent a subset of possible M ode-5 failure responses. Random-attitude failures can be used to establish the maximum possible region of impact, given that a vehicle has flown normally for a specified period of time. For this purpose RTI has developed a Random-A ttitude Failure Impact Point (RA FIP) program written in Fortran (3900 lines of code) for execution on a personal computer. U sing a M onte C arlo approach, program RA FIP first selects a starting time and then a random thrust direction on the attitude sphere, with all directions having the same chance of being chosen. Each M onte-C arlo run is begun using the nominal vehicle position and velocity at the selected start time, assuming an instantaneous change in thrust direction. Thrust is applied continuously in the selected random direction, and the equations of motion are numerically integrated until one of four conditions is satisfied: (1) final stage burnout occurs, (2) the vehicle impacts while thrusting, (3) orbital insertion occurs, (4) the vehicle breaks up due to aerodynamic forces For conditions (1) and (4), the trajectory is extended to impact using K epler's equations. For condition (3), an impact point does not exist The process just described is repeated 9/10/96 31 RTI for a suitably large sample so the distribution of resulting impact points will, for all practical purposes, represent all possible impact points, irrespective of the actual nature of the failure. D epending on vehicle breakup characteristics and failure time, a vehicle that experiences a random-attitude failure may break up at the instant of failure, or after a few seconds into the turn, or not at all. In making the calculations, three separate breakup thresholds and a no-breakup case were investigated. W ith respect to vehicle breakup, the assumption was made that the vehicle would break up if qa exceeded a specified constant limit, where q is the dynamic pressure and a is the total angle of attack. A lthough the breakup qa may well be a complicated function of M ach number and other parameters, this simplistic approach was taken. Random-attitude-failure calculations were made individually for A tlas, D elta, Titan, and LLV1 starting shortly after pitchover and continuing to some convenient time such as a stage burnout when the vehicle could no longer endanger the launch area. Theoretically, the M ode-5 impact density function extends downrange until the instantaneous impact point vanishes. Since this study is concerned with evaluation of density-function parameters for launch-area risk analysis, the random-attitude calculations were stopped at a staging event when the vehicle no longer had sufficient energy to return the impact point to the launch area. U sing trajectory data for each vehicle, program RA FIP was run to generate 10,000 impact-point samples at each starting time. C alculations were made at ten-second intervals. 6 .1.2 Slow-Turn Failures C ertain types of guidance and control failures can cause the thrusting engine to gimbal to null or a near-null position; Such failures can produce what is herein called a slow turn. For various reasons, after an engine is commanded to null it may not thrust precisely through the center of gravity, e.g., structural misalignments, shifting center of gravity, canted nozzles. Since, like random-attitude failures, slow turns constitute a subset of M ode-5 failure responses, they have been investigated using RTI program RA FIP. The following assumptions have been made in making the calculations: (1) The effective thrust offset of a "nulled" engine is normally distributed with a zero mean and a standard deviation of 0.1°. (2) A fixed thrust offset results in a constant angular acceleration of the airframe, and thus a constant angular acceleration of the thrust vector. (3) For small thrust misalignments, the angular acceleration of the airframe is proportional to the angular thrust misalignment. A t each time point, the angular acceleration produced by small thrust offsets was estimated from the malfunction turn data provided to the safety office by the range user. M alfunction turns for the A tlas H A S were provided for three gimbal angles, the smallest being one degree. For each gimbal angle, the results were plotted as 9/10/96 32 RTI cumulative angle turned versus time. Since the slope of the curve (i.e., the turning rate) is greatest when the thrust (and thus airframe) is directed at right angles to the velocity vector, the average angular acceleration during the first 90° of rotation was obtained from the equation 0 = -012 (4) 2 so that t (sec ) t sec where t is the elapsed time from the beginning of the tumble turn until the airframe has rotated approximately 90°. If the assumption is made that the angular acceleration is directly proportional to the thrust offset angle (i.e., nozzle deflection), the angular acceleration 0d for any small deflection angle becomes % = 4 (6) o where 0 is the angular acceleration computed from Eq. (5) for deflection angle 8 (1° for A tlas H A S), and 8d is some small deflection angle. U sing the A tlas H A S data, angular accelerations 0 were computed at ten-second intervals from the programming time of 15 seconds to 275 seconds for 8 = 1°. For each starting time, a normal distribution with zero mean and a standard deviation of 0.1° was sampled to obtain an initial thrust misalignment 8d to substitute in Eq. (6). The resulting angular acceleration 0d was applied throughout the turn. Slow-turn calculations were made in a manner analogous to the random-attitude turns, using the reference trajectory to obtain the starting position and velocity components. The slow turn was assumed to occur in a randomly oriented plane containing the starting velocity vector. Each turn was carried out until one of the four conditions listed in Section 6.1.1 for random-attitude turns was met. For conditions (1) and (4), impact points were calculated and, along with thrusting impacts from condition (2), summed for each five-degree sector from 0° to 175°. A t each starting time, 10,000 impact-point calculations were made. 6 .1.3 Factors Affecting Malfunction-Turn Results Random-attitude turns and slow turns are only subsets of the totality of M ode-5 failure responses. A s discussed earlier in Section 3, other types of behavior following a M ode- 5 failure are numerous and largely impossible to categorize, much less simulate. Ideally, impact distributions from all types of M ode-5 responses should be combined before results are compared with those obtained from the theoretical M ode-5 impact 9/10/96 33 RTI density function. Since this could not be done in general, impacts from only the two types of malfunction turns were considered. Several factors affect the results of the simulations: a. W eighting of turn data: Both random-attitude and slow-turn simulations were made for A tlas H A S. In combining impacts from the two data sets, random­ attitude turns were assumed to be three times as likely to occur as slow turns. A factor of three was selected since, among the M ode-5 failure responses in the performance summaries for A tlas, D elta, and Titan, random-attitude turns appeared to occur about three times as often as slow turns. In many cases, lack of detailed information made it difficult to' decide whether a M ode-5 response should be considered as a random-attitude turn, a slow turn, or some other type of failure. The relative weighting of turns makes little difference, however, since the impact distribution for the two types of turns are similar (as shown later in Figure 5), and since the weighted composite must lie between the two. It was assumed that similar results would be obtained for D elta, Titan, and LEVI, so slow-turn computations were not made for these vehicles, cutting the number of time-consuming simulations in half. b. Breakup qa: In the turn calculations, the assumption was made that vehicle breakup would occur if a certain value of qa was reached. In addition to the no­ breakup case which is considered unrealistic, separate runs were made for three constant values of qa: 5,000, 10,000, and 20,000 deg-lb/ft2. A s stated previously, the determination of vehicle breakup is, in reality, much more involved than this simplistic approach would suggest. H owever, to add realism to the malfunction­ turn calculations, use of a simple approach seemed better than none at all. For Titan IV, allowable (but not breakup) qa's were provided as functions of M ach number. The maximum permissible value and corresponding M ach number for Titan/C entaur, Titan/NU S, and Titan/IU S were, respectively, 6819 deg-lb/ft2 at M ach No. 0.77, 5332 deg-lb/ft2 at M ach No. 0.815, and 17,000 deg-lb/ft2 at M ach No. 0.325. For A tlas, D elta, and LLV1 vehicles, no breakup qa data were available. The breakup qa's used in the calculations bracket the range of permissible qa's for the Titan vehicles. c. End time TB: The simulated impact distributions from random-attitude failures and slow turns were compared with impact distributions computed from the M ode-5 theoretical impact-density function. For the comparisons to be meaningful, the value selected for TB in the M ode-5 impact-density equation and the stop time for thrusting-turn simulations must be the same. To some extent, the shaping constants A and B derived by fitting the theoretical and simulated impact data depend on T^ since the percentage of impacts in each 5° sector depends on TB. H owever, after A and B have been established for a particular T„ using a different TB in the D A M P calculations has no effect on computed risks provided an adjustment is made in the probability of occurrence of a M ode-5 9/10/96 34 RTI response. Referring to Eq. (3), the right-hand member must be multiplied by the probability p5 of a M ode-5 response to obtain absolute probabilities. Except for TB itself (and to a slight degree, shaping constants A and B), the quantities in the equation do not depend on TB. Thus if TB and p5 are both changed so that p5/(TB - Tp) remains constant, the computed risks are unchanged. If destruct action (i.e., impact limit lines) is included in the D A M P calculations, the supplemental risks* resulting from that action must be accounted for. In this case, die termination time has a minor influence on results, since it affects the number of impacts that would occur beyond the impact limit lines without destruct that are forced inside when destruct action is taken. If destruct action is omitted, the value of TB is immaterial (i.e., supplemental M ode-5 risks are non­ existent) provided that the impact range along the reference trajectory at time TB exceeds the range to all targets of interest. (Except in this paragraph, supplemental M ode-5 risks are not addressed in this present report.) * See Ref. [1], Section 10. d. Vacuum calculations: A tmospheric effects were accounted for in determining when vehicle breakup would occur and, to some extent, during each thrusting turn by using accelerations from the nominal trajectory. To reduce computer time and cost of this study, vacuum calculations were made during free fall after vehicle breakup or burnout. A lthough this increased impact dispersions somewhat, vacuum results should not be drastically different from those obtainable using a maximum-beta piece. In theory at least, different mode-5 shaping constants exist for each debris class. In view of the uncertainties in vehicle breakup conditions and characteristics, and in the overall process of simulating M ode-5 malfunctions, attempts to derive unique shaping constants for each debris class did not seem justified. 6 .1.4 Malfunction-Turn Results for Atlas H AS For A tlas H A S, the distribution of impacts for simulated random-attitude turns, slow turns, and a weighted combination (75% random-attitude and 25% slow turn) are shown in Figure 5. Since the impact distribution (i.e., the percentages of impacts in 5° sectors) for the weighted composite was not significantly different from that for random-attitude failures, slow-tum computations were not made for D elta, Titan, and LLV1. 9/10/96 35 RTI Figure 5. C ombined Random-A ttitude and Slow-Turn Results 9/10/96 36 RTI 6 .2 Shaping Constants for Atlas H AS 6 .2.1 Optimum Mode-5 Shaping Constants Since the dynamic pressures that can cause the A tlas H A S to break up were not available, random-attitude failures were simulated for a no-breakup case and for three breakup qa's: 20,000 deg-lb/ft2, 10,000 deg-lb/ft2, and 5,000 deg-lb/ft2. For each case, 270,000 trajectories were run, giving a total of 1,080,000. It turned out that the value chosen for the breakup qa was critical in determining shaping constant A , since the lower the qa, the less the thrusting time before breakup, and the higher the percentages of impacts in sectors near the flight line. For A tlas H A S, the effects of qa on breakup are shown in Figure 6 where, for the selected qa's, the percentages of random-attitude turns that result in breakup before 280 seconds are plotted against failure time. Figure 6. A tlas H A S Breakup Percentages for Random-A ttitude Turns For failures between 10 and 30 seconds, most breakups do not occur at failure, but later in flight after the vehicle has built up significant velocity. For failures between 40 and 105 seconds, more than 80% breakup occurs, even for qa's as high as 20,000 deg-lb/ft2. 9/10/96 37 RTI In this region, breakup occurs at or shortly after vehicle failure. Beyond 170 seconds, the dynamic pressure between failure and 280 seconds stays sufficiently low so that the vehicle remains intact. The dramatic differences in impact distributions that can result at certain times during flight if the vehicle is subject to aerodynamic breakup can be seen by comparing the impact footprints in Figure 7 and Figure 8. Both patterns show 10,000 impact points from random-attitude failures of the A tlas H A S at 130 seconds. Figure 7 is for no breakup, and Figure 8 is for a breakup qa of 5,000 deg-lb/ftz. The data in Table 19 comprise an example of a 270,000-point sample of random-attitude failures run at 10-second intervals from 15 to 275 seconds. (For brevity, only every- other failure time is shown in the table.) Ten thousand impacts are computed at each failure time. Five-degree sectors are identified in the left-hand column. For each time, the number of impacts in each 5° sector is shown in the column for that time. The total number of impacts for all failure times and the percentages of impacts in each sector are given in the last two columns of the table. 9/10/96 38 RTI Figure 7. A tlas H A S Impacts with No Breakup 9/10/96 39 RTI Figure 8. A tlas H A S Impacts with Breakup £ co o Z £ tn < CD < a o •43 i B « CL £M (U 'CL £ H CD 3 LncN®Ln(MOinHOCh’sOM*^cncMCMHOOOas^CsOOCiOOOOOOONNNNNNNN d^N^CncndddHHHHrHHriHHHHQQQQQQddQQOdoddd CO H o o § 3^^^c\^ooa>ooa\x^o(^|\ooo(NNooNr^(N^^^(^lcn^(N^c^QlnQrtH b3fMHooHoo»m(NinQ»\o5cnooohoo'Oin^ncncMNm MOO^N\C^DmmM<^COC^(M(NCMNHHHHHHHH 8 in ChOtxCMin\OCMinQQM3CMi-iahChxOCOCOr-HN\ooooooinaMnLnosH CMCMCMCMCMCMCMCMCMCMCMCMCMCMCMCMCMCMCMCOCMCMCMCMCOCMCMCMCMCOCMCMCMCNCMCO o o 8 c? < OLnomomomQLnomomomomomomomoLCjQmQinomomom HHtNn^cn^^inLn'sO^NNxxox^ooHHCNcjcn^J^^^^^^^ 1 9 /10/9 6 41 RTI In Figure 9, the percentages of impacts in 5° sectors from 0° to 180° have been plotted for A tlas IIA S random-attitude turns out to 280 seconds. (It should be remembered that random-attitude turns are representative of combined random-attitude and slow turns.) For B = 1000, theoretical M ode-5 impact percentages are also plotted in the figure for best-fit values of A obtained by trial and error. Figure 9. A tlas IIA S Simulation Results with B = 1,000 By observing curve shapes, it can perhaps be seen that no single value of A causes a theoretical impact distribution and a distribution of impacts from random-attitude turns to match closely over the entire range of 5° sectors. A ttempts to improve the match on one end of the curve by selecting a different A merely degrades the match on 9/10/96 42 RTI the other end. It is possible, however, to obtain fairly close agreement over sectors* from ±80° to ±180°, as seen in Figure 9. Since for A tlas H A S there are few, if any, significant population centers in the launch area outside these sectors (i.e., within ±80° of the flight line), failure of the curves to match closely near the flight line is of little consequence. If a better data match is considered desirable for computing risks to population centers within ±80° of the flight line (e.g., ships), either a different A can be selected for use with B = 1,000 or other values of A and B can be derived. If only a single value of B is used, no matter what the value, a good match between theoretical and simulated data is not possible over the entire 180° sector for various breakup qa's. * For other values of B and qa, dose agreement is possible from ±60° to ±180°. Before becoming too concerned about lack of a data match between 0° and 80°, it should be remembered that many types of M ode-5 responses cannot be simulated, so that the malfunction-turn impact distributions plotted in Figure 9 are only a subset of all possible M ode-5 impacts. Based on twelve M ode-5 failure responses for which impact data are available, it is believed that inclusion of the "non-simulatable" M ode-5 responses would considerably improve the match in the sector from +10° to ±80°. A nother mitigating factor is that risks near the flight line are totally dominated by M ode-4 failure responses. To see how data matching is affected by selecting widely differing values of B, the theoretical M ode-5 impact distributions were computed for B = 50,000,100,000,500,000, and 5,000,000. Best-fit values for A were again determined by trial and error. Results are shown in Figure 10 through Figure 13 along with the same impact distributions for random-attitude turns plotted in Figure 9. 9/10/96 43 RTI 0 20 40 6 0 80 100 120 140 16 0 180 Angle From Flight Path (deg) Figure 10. A tlas H A S Simulation Results with B = 50,000 9/10/96 44 RTI Angle From Flight Path (deg) Figure 11. A tlas ILA S Simulation Results with B = 100,000 9/10/96 45 RTI 0 20 40 6 0 80 100 120 140 16 0 180 Angle From Flight Path (deg) Figure 12. A tlas ILA S Simulation Results with U = 500,000 9/10/96 46 RTI 0 20 40 6 0 80 100 120 140 16 0 180 Angle From Flight Path (deg) Figure 13. A tlas H A S Simulation Results with B = 5,000,000 9/10/96 47 RTI The five values of B and the corresponding best-fit values of A used to compute the M ode-5 distributions shown in Figure 9 through Figure 13 are tabulated in Table 20. It is apparent that the value of A is dependent on both qa and B. In general, if a larger value of B is selected, a larger value of A is required to effect a fit with the random­ attitude-turn data. On the other hand, if the breakup qa is increased, the required value of A must be decreased. Only qa is critical since, as shown later, any value of B, together with its corresponding value of A , can be used in the launch-area risk computations if significant targets do not lie within ±80° of the flight line. Table 20. Shaping C onstants for A tlas H A S Breakup qa (deg-lb/ft2) B A none 20,000 14,000 * 10,000 5,000 1,000 1.90 2.75 3.00* 3.20 3.45 none 20,000 10,000 5,000 50,000 3.15 4.10 4.50 4.75 none 20,000 10,000 5,000 100,000 3.40 4.30 4.75 5.00 none 20,000 10,000 5,000 500,000 4.00 4.85 5.30 5.55 none 20,000 10,000 5,000 5,000,000 4.75 5.65 6.10 6.30 * interpolated 9/10/96 48 RTI Because of the uncertainties in breakup conditions, the values of A for each B in Table 20 have been plotted against qa in Figure 14. By reading from the plots, a value of A for the five values of B can be obtained for any breakup qa deemed appropriate between 5,000 and 20,000 deg-lb/ft2. Figure 14. Effects of Breakup q-alpha on A for A tlas H A S 6 .2.2 L aunch-Area Mode-5 Risks The twenty sets of A and B shown in Table 20 were used to compute M ode-5 launch­ area risks for population centers inside the impact limit lines for an A tlas ILA S daytime launch of a Telstar-4 payload from Pad 36A . Results of these and two other cases are given in Table 21. The M ode-5 Ec in the first line (old baseline case) of Table 21 is presented for comparison only. It was obtained from data in the first line of Table 45 of an earlier RTI study01. In Ref. [3], the total A tlas H A S failure probability for the first two minutes of flight was set at 0.04, with the probability of a M ode-5 failure response assumed to be 0.005. The second line in Table 21 shows the result of a recomputation of the M ode-5 baseline risks, again with B = 1000 and A = 3, using newly derived values for the total failure probability and for a M ode-5 failure response. For flight phases 0 - 2, a total failure probability of 0.031 was assumed, as extracted from Table 6 for 9/10/96 49 RTI F = 0.98. The conditional probability of a M ode-5 response was assumed to be 0.08 (from the last line of Table 15), so the absolute probability was 0.031 x 0.08 = 0.0025. For the remaining cases in Table 21, the same assumptions were made for the total failure probability and for the probability of a M ode-5 response. * Interpolated from Figure 14 Ta?le 21. Shaping C onstants and Related Risks for A tlas IIA S Ps T X B (sec) Breakup qa (deg-lb/ft2) B A M ode-5 Ec (x 10^) 0.005 118 14,000 * (baseline) 1,000 3.00 227 0.0025 280 14,000 * (newp5 & Tb) 1,000 3.00 49.1 0.0025 280 none 20,000 10,000 5,000 1,000 1.90 2.75 3.20 3.45 139.8 73.7 33.4 19.8 0.0025 280 none 20,000 10,000 5,000 50,000 3.15 4.10 4.50 4.75 144.9 75.6 37.1 21.8 0.0025 280 none 20,000 10,000 5,000 100,000 3.40 4.30 4.75 5.00 144.8 79.8 36.1 21.1 0.0025 280 none 20,000 10,000 5,000 500,000 4.00 4.85 5.30 5.55 143.6 79.9 35.9 20.8 0.0025 280 none 20,000 10,000 5,000 5,000,000 4.75 5.65 6.10 6.30 144.8 77.7 34.2 22.0 A s seen from Table 21, the M ode-5 risks are highly dependent on A and insensitive to the value chosen for B provided a proper choice is made for A . Even for values of B as different as 1,000 and 5,000,000, the M ode-5 risks (qa = 5,000) differ by only 12% . This difference drops for all other values of B. In fact, the differences probably have more to do with the choice of A than to any inherent difference in results due to the choice of B. For A tlas IIA S, 24% of the total M ode-5 Ec in the launch area is due to one population center, and 51% of the total Ec to only five population centers (see page 49 of Ref [3]). If values of A had been chosen so that theoretical distributions and random-attitude-turn distributions more nearly matched for the radial directions to these population centers, 9/10/96 50 RTI the differences in calculated M ode-5 risks for the different values of B would surely have been less. Further understanding of why small differences in Ec exist can be gained by plotting values of the M ode-5 density function computed from Eq. (3) This has been done in Figure 15 for a range of three miles using values of A and B from Table 21 for qa = 5,000 deg-lb/ft2. Since Eq. (3) does not include a factor to account for the probability of a M ode-5 failure, the values plotted in the figure are conditional impact probabilities per square mile. For the sector from 120° to 180°, which is where most population centers are located, the density-function value for B = 5,000,000 is largest and for B = 1,000 is smallest. Results consistent with this are shown in Table 21, where the largest and smallest E^s are for B = 5,000,000 and B = 1,000, respectively. Theta (deg) Figure 15. M ode-5 D ensity-Function Values at Three M iles 6 .2.3 Effects of Mode-5 Constants on Ship-H it Contours In the preceding section, certain values were assigned to B and, by trial and error, best- fit values of A were found. For every breakup qa and every B, it was possible to find a value of A that produced good agreement between theoretical and simulated impact data over 5° sectors from ±100° to ±180° (see Figure 10 through Figure 13). In some 9/10/96 51 RTI cases the agreement gradually deteriorated for angles below ±100° while, in other cases, agreement was remarkably good to ±40°. Below this, agreement was generally poor except in a region between ±3° and ±6° where the theoretical and simulated curves crossed. A s pointed out previously, for A tlas pad locations at the C ape essentially all significant population centers (except ships) are located in the sectors from ±100° to ±180°. Thus any B with the corresponding best-fit value of A can be used to compute launch-area risks, irrespective of the assumed breakup qa. In unusual cases at the C ape or at other launch locations, population centers may be located outside sectors of good agreement for some B's. If such situations arise, a value of B should be used in the risk calculations that produces the best fit over the largest sector possible, generally ±40° to ±180°. The values of B producing this result are listed in Table 22 as functions of breakup conditions. Table 22. Best-Fit C onditions for A tlas H A S J Breakup C onditions B A none 50,000 3.15 20,000 100,000 4.30 10,000 100,000 4.75 5,000 5,000,000 6.30 A lthough the selected values of A produce poor agreement in the sectors from 0° to ±40°, this does not mean that good agreement in this region is impossible. Instead, it means that the value of A required to produce good agreement in the ±40° sectors will produce poor agreement elsewhere. In special situations where the only population centers of interest are within ±40° of the flight line, other values of A can be derived for use in the risk calculations. From a practical standpoint, the effort required to find a value of A that produces a better fit within1 ±40° or so of the flight line is unnecessary. W ithin this sector, the M ode-4 failure response, which is almost 11 times more likely to occur than a M ode-5 response, totally dominates the computed risks. A s verification, the D A M P program was run for the A tlas H A S vehicle, and ship-hit contours plotted for three vastly different pairs of A 's and B's. The results are shown in Figure 16 through Figure 21, where the total failure probability during the first two minutes of flight was assumed to be 0.04, and the probabilities of M ode-4 and M ode-5 responses were 0.033 and 0.005, respectively: For each A and B, ship-hit contours were computed for M ode 5 alone, and then for all response modes. A s expected, some downrange extension occurred in the M ode-5 contours as the value of A was increased, since the higher the value of A , the more concentrated impacts are near the flight line. W hen all response modes were included in the calculations, contour differences were almost imperceptible, showing the total dominance of M ode 4. If the calculations were remade with a M ode-4 9/10/96 52 RTI response 10.9* instead of 6.6 (0.033 + 0.005 = 6.6) times as likely as a M ode-5 response, the differences in contours would be even less. * From Table 15,86.2 + 7.9 = 10.9. 15 Atlas IIAS 10^ 10 Mod0 5 P| 10 + (D O) c -io B = 1,000 A = 3.b0 -15 -5 0 5 10 15 20 25 D ownrange D istance (nm) Figure 16. A tlas H A S M ode-5 Ship-H it C ontours with A = 3.00 9/10/96 53 RTI Figure 17. A tlas H A S A ll-M ode Ship-H it C ontours with A = 3.00 9/10/96 54 RTI AtladllAS B = 1,000 A = 3^5 -5 0 5 10 15 20 25 D ownrange D istance (nm) Figure 18. A tlas IIA S M ode-5 Ship-H it C ontours with A = 3.45 9/10/96 55 RTI Figure 19. A tlas IIA S A ll-M ode Ship-H it C ontours with A = 3.45 9/10/96 56 RTI 15 Atlas H AS 10l w6 Mod6 5 P 10 b 0 c -10 B = 5,000,000^ A = 6 b0 -15 -5 0 5 10 15 20 25 D ownrange D istance (nm) Figure 20. A tlas H A S M ode-5 Ship-H it C ontours with A = 6.30 9/10/96 57 RTI Figure 21. A tlas IIA S A ll-M ode Ship-H it C ontours with A = 6.30 6 .2.4 Range D istributions of Theoretical and Simulated Impacts Earlier discussions had to do with how well the angular part of the M ode-5 impact density function could be made to agree with angular data derived from simulated random-attitude turns. A similar procedure was used to- test agreement between the range part of the M ode-5 impact density function and the simulated data. For this purpose, beginning at 15 seconds random-attitude turns were made at 2-second intervals out to 279 seconds, assuming no breakup and breakup qa's of 5,000 and 20,000 deg-lb/ft2. A t each time, 2,000 trajectories and impact points were computed, giving a total sample of 266,000 for each breakup condition. For each impact point, the range from the pad was computed, and the total number of impacts calculated in 10- mile range intervals out to 350 miles. Impacts beyond this range were placed in a single range category. The percentage of impacts in each range interval was then computed and plotted as shown in Figure 22. 9/10/96 58 RTI Figure 22. Impact-Range D istributions Theoretical impact percentages for the same 10-mile range intervals were obtained by integrating the M ode-5 impact-density function [Eq. (3)] between the angle limits of zero and k, and between the range limits of ^ and R,, and doubling the results. The percentages are plotted in Figure 22. A s pointed out in more detail at the end of A ppendix B, the percentage of impacts in any range interval is independent of the values of A and B. Figure 22 shows that the range impact distributions for theoretical M ode-5 impacts and random-attitude failures for breakup qa's between 5,000 and 20,000 deg-lb/ft2 are in excellent agreement out to 50 miles. Theoretical percentages and random-attitude percentages for qa = 5,000 deg-lb/ft2 (considered to be the most realistic value) are in good agreement out to 190 miles. Beyond that the differences appear fairly large, magnified as they are by the logarithmic scale, although the maximum absolute difference is only 0.4% . The steep rise in all curves at 350 miles is artificially created by lumping all impacts beyond 350 miles into one range interval instead of 10-mile intervals. 9/10/96 59 RTI 6 .3 Shaping Constants for D elta-GEM A lthough less extensive, the computations made and graphs plotted to establish M ode- 5 shaping constants for D elta parallel those described in Section 6.2 for A tlas H A S. The approach may be summarized as follows: (1) C alculate impact points from 10,000 simulated random-attitude turns made at 10- second intervals from programming time at 6 seconds until staging at 270 seconds (260,000 simulations total). The impact points from these turns, which produce impact results similar to slow turns, are assumed to be representative of the totality of M ode-5 impacts. (2) D etermine the percentages of impacts in 5° sectors from 0° to 180°. (3) For assumed values of A and B, compute the percentages of impacts in the same 5° sectors from the theoretical M ode-5 impact-densityfunction. (4) By trial and error, find values of A and B that provide a best fit between the simulated and theoretical impact data. 9/10/96 60 RTI 6 .3 .1 Optimum Mode-5 Shaping Constants The percentage of D elta vehicles that break up during simulated random-attitude turns are plotted against failure time in Figure 23. The same breakup qa's used in the A tlas IIA S calculations were used here. It can be seen from the figure that over 50% of the vehicles break up, either immediately or eventually, if a turn begins between about 10 and 115 seconds. Figure 23. D elta-G EM Breakup Percentages 9/10/96 61 RTI Figure 24 shows the percentages of malfunction-turn impacts in 5° sectors for no breakup and for breakup qa's of 20,000, 10,000, and 5,000 deg-lb/ft2. For B = 1,000, theoretical M ode-5 impacts are also plotted using best-fit values of A . This value of B was chosen since it is currently used by RTI in making launch-area risk studies for the 45th Space W ing. In the sectors from ±80° to ±180°, where most of the population centers are located, fairly good data fits were possible for all breakup qa's except 5,000 deg-lb/ft2. No value of A could be found to produce a good fit with B = 1,000. The bottom plot in Figure 25 shows that an excellent fit between malfunction-turn and theoretical data is possible for qa = 5,000 deg-lb/ft2 if a different choice of B is made. Figure 24. D elta-G EM Simulation Results with B = 1,000 9/10/96 62 RTI The simulated impact percentages plotted in Figure 25 are identical with those shown in Figure 24. The theoretical percentages in Figure 25 were obtained by trying various combinations of B and A until the best possible fit was obtained in the sectors from ±60° to ±180°. From these plots it seems apparent that a reasonable fit between malfunction­ turn and theoretical M ode-5 impact data can be found for any qa between 5,000 and 20,000 deg-lb/ft2. 0.01-------- L-------i1ii'-------- 0 20 40 6 0 80 100 120 140 16 0 180 Angle From Flight Path (deg) Figure 25. D elta-G EM Simulation Results with Best-Fit Shaping C onstants 9/10/96 63 RTI 6 .3 .2 L aunch-Area Mode-5 Risks U sing values of A and B from Figure 24 and Figure 25, program D A M P was run to compute M ode-5 launch-area risks for population centers inside the impact limit lines for a D elta-G EM /G PS-10 daytime launch from Pad 17A . Results from these and two other cases are shown in Table 23. The M ode-5 Ec in the first line (old baseline case) is presented for comparison. It was obtained from the first line of Table 55 of an earlier RTI study®. In that study, the total D elta failure probability during the first 130 seconds of flight was set at 0.02, with the probability of a M ode-5 response assumed to be 0.0025. The second line in Table 23 shows the result of a recomputation of the M ode- 5 risks, again with B = 1,000 and A = 3, using failure probabilities derived earlier in this report. From Table 6 and Table 15, the failure probability during flight phases 0 - 2 is 0.013, and the relative frequency of occurrence of a M ode-5 response is 0.08. The absolute probability of a M ode-5 response thus becomes 0.013 x 0.08 = 0.001. Tab e 23. Shaping C onstants and Related Risks for D elta-G EM ______ T XB (sec) Breakup qa (deg-lb/ft2) B A M ode-5 Ec (x 10*) 0.0025 . 130 12,000 * (baseline) 1,000 3.00 394 0.001 270 12,000 * (new p5 & Tb) 1,000 3.00 88.8 0.001 270 none 1,000 1.90 220.0 20,000 2.90 104.4 10,000 3.10 74.1 5,000 4.30 5.2 0.001 270 none 10,000 2.60 224.4 20,000 2,000 3.15 102.4 10,000 2,000 3.35 72.0 5,000 4 3.50 5.1 * Interpolated from data contained in Figure 24 A s in the case of A tlas, Table 23 again shows that the risks in the launch area are highly dependent on qa and thus on A , but relatively insensitive to changes in B if a proper value is selected for A . For example, if qa = 10,000, the computed risks for B = 1,000 (A = 3.10) and B = 2,000 (A = 3.35) differ byTess than 3% . For the no-breakup cases where B = 1,000 and then 10,000, the computed risks in the launch area differ by less than 2% . Launch-area risks are highly dependent on the vehicle's capability to withstand aerodynamic forces. Except early in flight, low-strength vehicles generally break up quickly after a malfunction turn begins. The later such turns occur, the more likely pieces are to impact downrange of the launch point, thus lessening risks to uprange populations. The effects of vehicle strength on risk are clearly seen in Table 23 where, 9/10/96 64 RTI for example, the risks are over 20 times as great if the vehicle's breakup qa is 20,000 rather than 5,000 deg-lb/ft2. 6 .4 Shaping Constants for Titan IV M ode-5 shaping constants for Titan IV were developed as described in Section 6.3 for D elta, except that a total of 290,000 simulations were run between the programming time of 18 seconds and staging at 300 seconds. The percentage of vehicles that break up during simulated random-attitude turns are plotted against failure time in Figure 26. The same qa's used with A tlas and D elta were used here, and similar breakup results were obtained. Figure 26. Titan IV Breakup Percentages 9/10/96 65 RTI Figure 27 shows the percentages of malfunction-turn impacts in 5° sectors for no breakup and for breakup qa's of 20,000, 10,000, and 5,000 deg-lb/ft2. For B = 1,000, theoretical M ode-5 impact distributions are also plotted in the figure using best-fit values of A . This value of B was chosen since it is currently used by RTI in making launch-area risk studies for 45 SW /SE. W ithin the sectors from ±60° to ±180°, where most population centers are located, data fits are reasonably good. A s seen in the next figure, the divergence for the no-breakup case can be greatly reduced by selecting other values for B and A . Figure 27. Titan Simulation Results with B = 1,000 9/10/96 66 RTI m w O ^; Figure 28. Titan Simulation Results with Best-Fit Shaping C onstants w P 9 m 8 fl) p I p w £ O 3 p s O 2 3 0)W m 8 w O 3 O C D (D O o w p 3 fD § P nT ti p > c 3 p ORO I fl) 3 fl) W I p o 9 P s o m m a OR fl) w 3 mm o P 3 Q. ^ 2 < ^ 2 3 S w 3 ff o o a> S’ fl) M oo p 3 fl) 3 p o r w fl) S' o 3 The best-fit values of B and A shown in Figure 27 and Figure 28 are tabulated for convenient reference in Table 24. For breakup qa's of 10,000 and 5,000 deg-lb/ft2, the currently-used value of B = 1,000 provided a better data fit than other values of B that were investigated. Table 24. Shaping C onstants for Titan IV T (sec) Breakup qa (deg-lb/ft2) B A 300 none 20,000 10,000 5,000 1,000 2.00 2.95 3.25 3.50 300 none 20,000 10,000 5,000 10,000 2,000 1,000 1,000 2.70 3.15 3.25 3.50 Risk calculations in the launch area were not made for Titan IV. 9/10/96 68 RTI 6 .5 Shaping Constants for L L V1 Shaping constants for LLV1 were developed as described in Section 6.3 for D elta, except that a total of 290,000 simulations were made between the programming time of 1 second and staging at 290 seconds. The percentages of vehicles that break up during simulated random-attitude turns are plotted in Figure 29. A s expected, the results are similar to those shown previously for A tlas, D elta, and Titan although, due to its higher acceleration, the rapid drop-off from near 100% breakup occurs at an earlier time for the LLV1 than for the other vehicles. Figure 29. LLV1 Breakup Percentages 9/10/96 69 RTI Figure 30 shows the percentage of malfunction-turn impacts in 5° sectors for no breakup, and for breakup qa's of 20,000, 10,000, and 5,000 deg-lb/ft2. The three breakup qa's produced impact distributions that were surprisingly similar, possibly due to the vehicle's higher acceleration. Theoretical M ode-5 impact distributions are also plotted in the figure for B = 1,000 and best-fit values of A . This value of B was chosen since it is currently used by RTI in making launch-area risk studies for 45 SW /SE. For all except the no-breakup case, values of A were found that produced good fits between the malfunction-turn and M ode-5 impact distributions in the sectors from ±60° to ±180°. Figure 30. LLV1 Simulation Results with B = 1,000 9/10/96 70 RTI Figure 31 shows that a good fit for the no-breakup case is possible if higher values of B and A are used. The simulated malfunction-turn impact distributions for the breakup cases plotted in this figure are identical with those in Figure 30. Since the theoretical percentages for B = 1,000 produced excellent fits, these values were simply replotted in Figure 31. For the no-breakup case, various combinations of B and A were tried before arriving at the plot shown in the figure. Figure 31. LLV1 Simulation Results with Best-Fit Shaping C onstants 9/10/96 71 RTI The best-fit values of B and A from Figure 30 and Figure 31 have been listed for convenient reference in Table 25. It is interesting to note that, for all breakup conditions, the currently-used value of B = 1,000 provided a better data fit than any other B that was investigated. Tab e 25. Shaping C onstants for LLV1______ Il T (sec) Breakup qa (deg-lb/ft2) B A 290 none 20,000 10,000 5,000 1,000 1.85 2.60 2.70 2.75 290 none 20,000 10,000 5,000 10,000 1,000 1,000 1,000 2.45 2.60 2.70 2.75 No launch-area risk calculations were made for LLV1. 6 .6 Shaping Constants for Other L aunch Vehicles Procedures for developing M ode-5 shaping constants A and B are fully described in this report. For A tlas, D elta, Titan, and LLV1, best-fit values of A were derived for four breakup conditions (1) for the currently-used value of B = 1,000, and (2) for optimum-fit values of B. For any new launch vehicle requiring risk calculations, the same procedures should be followed to obtain suitable values for A and B. A s an alternative and less time-consuming process, values of A and B can be estimated by comparing the new vehicle with one of the four vehicles referred to above and listed in Table 26. If the configuration and trajectory of the new vehicle and one of the listed vehicles are similar, values of A and B shown in the table for that vehicle and the assumed breakup condition can be used. There may, of course, be no similarity between the new vehicle and any of the listed vehicles. In that event and depending on assumed breakup conditions, one of the mean values shown in the last row of the table can be selected until better values can be developed. Table 26. Summary of A Values for B = 1,000 IP Range (nm) Breakup qa (deg-lb/ft2) Vehicle at 30 sec 5,000 10,000 20,000 None A tlas H A S 0.3 3.45 3.20 2.75 1.90 D elta-G EM 5.2 4.30 3.10 2.90 1.90 Titan IV 1.9 3.50 3.25 2.95 2.00 II ELV1 33.4 2.75 2.70 2.60 1.85 || Other vehicles 3.5 3.1 2.8 1.9 9/10/96 72 RTI 7. Potential Future Investigations Because of contract limitations on funds and the deadline for publishing the report, certain interesting facets of the M ode-5 modeling process could not be fully investigated. Several such issues are listed below in considered order of importance: (1) Effects on shaping constants A and B of using more precise breakup (qa) conditions during malfunction-tum simulations. (2) Effects on shaping constants A and B (and thus overall risks) if different values of Tb are used in computing theoretical and simulated impacts (e.g., TB corresponding to burnout of zero, first, and second stages). (3) Effects on shaping constants A and B if drag is accounted for in computing free­ fall impact points after a malfunction turn. (Shaping constants could be determined for maximum, minimum, and intermediate ballistic coefficients, then interpolated for other values. This more accurate approach would ultimately require extensive modifications to D A M P.) (4) Effects on shaping constants A and B if sectors smaller than 5° are used to compare theoretical and simulated impact data (e.g., 1° or 2°). (5) Effects on relative failure probabilities for solid-propellant vehicles if unclassified solid-propellant vehicles or declassified test results are used in the historical data samples (e.g., Pershing, Polaris, Poseidon, Trident). Other tasks that should be performed at some point in the future include: (a) U pdate absolute failure probabilities for A tlas, D elta, Titan, and perhaps other vehicles. (b) D evelop suitable shaping constants A and B for new vehicles. (In this regard, see Section 6.6) < 9/10/96 73 RTI 8. Summary In RTFs risk-computation program D A M P, vehicle failures per se are not considered. Instead each catastrophic failure is assumed to' produce one of five failure responses, and it is these response modes that are modeled in D A M P. A lthough most catastrophic failures result in impacts near the flight line, less likely malfunctions may cause debris to fall either uprange or well away from the flight line. In D A M P, vehicle failures with this potential are, for the most part, classified as M ode-5 failure responses. The resulting impacts are modeled by a rather formidable-looking density function that includes two shaping constants (A and B) that strongly influence the nature of the impact-density function. To obtain absolute probabilities (or risks), the function must be multiplied bya probability-of-occurrence factor (p5). The primary purpose of this study was to determine the best values for A , B, and p5 for various vehicle programs. Other objectives not explicitly included in the statement of work were to develop absolute failure probabilities for A tlas, D elta, and Titan and to derive relative probabilities of occurrence for the five failure-response modes in D A M P. A lthough some risk analyses may ignore unlikely failure-response modes, Section 2 demonstrates the need for a M ode-5 response - or some similar response - through brief descriptions of actual vehicle flights. Sections and A ppendixB provide the reader with a fuller understanding of the nature and intricacies of the M ode-5 impact­ density function. Together, they show how density-function shaping is affected by values of A and B, and in particular how the A tlas H A S launch-area risk contours change if the value of A is changed. Section 4 is a philosophical discussion of methods of assessing vehicle failure probability (or reliability). Two approaches are discussed, one strictly empirical, the other a parts-analysis method that involves the assignment of failure probabilities to individual parts, components, and systems. A lthough difficulties exist with both approaches, the empirical method was chosen to estimate both absolute and relative failure probabilities. A s the first step in estimating failure probabilities empirically, performance histories were gathered, summarized, and tabulated (A ppendix D ) by launch date for A tlas, D elta, and Titan vehicle launches from the Eastern and W estern Ranges, and for Thor launches from the Eastern Range. Obtaining this information, and assigning response modes and associated flight phases for each failure consumed a large portion of the effort expended on this task. A filtering (i.e., data weighting) technique was selected (see Section 5.1 and A ppendix C ) and applied to the launch failure data to estimate overall failure probabilities by flight phase (see Section D .1.3) for A tlas, D elta, and Titan vehicles. The recommended failure probabilities are based on test results involving only those vehicle configurations that are considered to be representative of current launch 9/10/96 74 RTI configurations (see Section D .L4). The results, summarized previously in Table 6 of Section 5.1, are repeated here in Table 27. Flight phases 0 - 1 go from liftoff through first-stage or booster cutoff, while flight phase 2 extends through second-stage or sustainer cutoff. A lthough failure probabilities for all flight phases are listed in Table 2, only malfunctions during flight phases 0 through 1 have significant effects on launch­ area risks. Table 27. Failure Probabilities for A tlas, D elta, and Titan Predicted Failure Probability Vehicle Flight Phase 0-1 Flight Phase 0-2 A tlas 0.022 0.031 D elta 0.010 0.013 Titan 0.040 0.064 A bsolute overall failure probabilities for A tlas, D elta, and Titan were based only on flight results from "representative" vehicle configurations. Because of the small number of failures in the individual representative samples, test results for all configurations (including Thor) were combined into a single sample and filtered to estimate relative failure probabilities for the five failure-response modes in program D A M P (see Section 5.2). The results for flight phases 0-2 and 0-1, together with recommended values for new launch systems, were summarized in Table 15 and Table 16, respectively, and are repeated here in Table 28 and Table 29. Table 28. Recommended Response-M ode Percentages for Flight Phases 0 -2 Response M ode M ature Launch Systems (F = 0.993) New Solid Systems (F = 0.996) New Liquid Systems (F = 0.999) 1 0.4 2.2 7.4 2 5.4 4.3 2.3 3 0.1 0.4 1.7 4 86.2 80.4 73.3 5 7.9 12.7 15.3 Table 29. Recommended Response-M ode Percentages for Flight Phases 0-1 Response M ode M ature Launch Systems (F = 0.993) New Solid Systems (F = 0.996) New Liquid Systems (F = 0.999) 1 0.5 3.4 10.7 2 7.4 6.6 4.3 3 0.1 0.6 2.4 4 81.9 74.5 67.0 5 10.1 14.9 15.6 For A tlas, D elta, and Titan, absolute probabilities for the individual response modes were obtained by multiplying absolute failure probabilities from Table 27 by the relative probabilities shown in the second columns of Table 28 and Table 29. The results, presented originally in Table 17, are repeated below in Table 30. To obtain 9/10/96 75 RTI these results, the relative probabilities used were more precise than those given in Table 28 and Table 29. No pretense is made that all figures in Table 30 are actually significant. Table 30. A bsolute Failure Probabilities for Response M odes 1-5 Vehicle: A tlas D elta Titan Flight Phase: 0-1 (0-170 sec) 0-2 (0-280 sec) 0-1 (0-270 sec) 0-2 (0-630 sec) 0-1 (0-300 sec) 0-2 (0-540 sec) || M ode 1 0.000119 0.000121 0.000054 0.000051 0.000216 0.000250 M ode 2 0.001637 0.001665 0.000744 0.000698 0.002976 0.003437 M ode 3 0.000011 0.000012 0.000005 0.000005 0.000020 0.000026 M ode 4 0.018007 0.026738 0.008185 0.011212 0.032740 0.055200 M ode 5 0.002226 0.002465 0.001012 0.001034 0.004048 0.005088 Total 0.022 0.031 0.010 0.013 0.040 0.064 The same chronological composite sample used to estimate relative failure probabilities for the failure-response modes was used to estimate the conditional probability that a M ode-3 or M ode-4 response terminates with a rapid tumble. This was found to be about one-third (see Section 5.3). Because the empirical data were insufficient to determine M ode-5 density-function shaping constants A and B, an alternate approach was used. Basically, for each of four vehicles (A tlas, D elta, Titan, and LLV1), M ode-5 failure responses were simulated at a series of failure times. The simulated malfunctions investigated were random-attitude turns and slow turns. A t each time, 10,000 impact points were computed. The percentages of impacts in 5° sectors from 0° (downrange) to 180° (uprange) were determined. These were compared with the percentages obtained in the same sectors from the theoretical M ode-5 impact-density function when specific values were assigned to A and B. By trial and error, values of A and B producing a good match between the two sets of percentages were established (see Section 6). A fter best-fit values were determined, the impact percentages for A tlas H A S in 10-mile range increments were checked to verify that the range part of the M ode-5 impact-density ■ function was consistent with impact ranges resulting from 266,000 simulated M ode-5 failure responses (see Section 6.2.4). Since the impact distributions resulting from simulated malfunction turns were highly dependent upon the dynamic pressure (qa) assumed to cause vehicle breakup, shaping constants A and B were likewise dependent on breakup assumptions. Three breakup qa's and a no-breakup case were investigated bysimulating 270,000 malfunction turns for each of the four conditions. A lthough a qa of 5,000 deg-lb/ft2 is considered most likely applicable for A tlas, D elta, and Titan, shaping constants for all breakup conditions were provided earlier in Section 6. 9/10/96 76 RTI Traditionally, a value of B = 1,000 has been used by the 45SW /SE in ship-hit calculations, and by RTI in performing launch-area risk analyses for the 45SW /SE. U sing this value of B, for each vehicle values of A were found that produced a good match between simulated and theoretical data. The results for qa = 5,000, 10,000, and 20,000 deg-lb/ft2 are given in Table 31. A s discussed earlier in the report, no single value of A could be found that produced a good fit over the entire 180° sector, although with one exception a good match did exist in the uprange portion of the sector from about ±90° to ±180°. For launches from C ape C anaveral, most population centers are located in this uprange sector. For any launch-area population centers located in the downrange sector, the risks are almost surely dominated by the M ode-4 failure response. Table 31. Summary of A Values for B = 1,000 Vehicle Flight Phase T XB (sec) Breakup qa (deg-]Lb/ft2) 5,000 10,000 20,000 A tlas IIA S 0-2 280 3.45 3.20 2.75 D elta-G EM 0-1 270 4.30 3.10 2.90 Titan IV 0-1 300 3.50 3.25 2.95 LLV1 0-2 290 2.75 2.70 2.60 Other vehicles — ... 3.5 3.1 2.8 Other values of B were investigated to find combinations of B and A that provided the best possible data fits over the largest possible portion of the 0° to 180° sector. A lthough no combinations of A and B could be found that produced good fits for the entire 180° sector, the values shown in Table 32 extended the fit from the uprange direction to within about 40° of the downrange direction. Table 32. Summary of Optimum M ode-5 Shaping C onstants Vehicle Flight Phase T X B (sec) Breakup qa (deg-lb/ft2) B A A tlas 0-2 280 5,000 5,000,000 6.30 D elta 0-1 270 5,000 4 3.50 Titan 0-1 300 5,000 1,000 3.50 LLV1 0-2 290 5,000 1,000 2.75 Launch-area risk calculations were made for A tlas and D elta to ascertain the effects of using radically different values of A and B in the M ode-5 impact-density function. For example, for a breakup qa of 5,000 deg-lb/ft2, values of A = 3.45 and B = 1,000 from Table 31 and A = 6.30 and B = 5,000,000 from Table 32 were used to determine total M ode-5 launch-area risks for an A tlas H A S launch from C omplex 36. The total risks differed by about 10% . (Other results for A tlas IIA S are given in Table 21, and for D elta in Table 23.) Other calculations for A tlas and D elta show that the value of B is not 9/10/96 77 RTI important in the launch-area risk calculations provided an appropriate value of A is selected. Since a good data match within ±40° of the flight line was not found, the effect of this on ship-hit calculations was investigated. It was discovered that the values chosen for A and B made no significant difference, since the risks to shipping near the flight line are totally dominated by the M ode-4 failure response (see Section 6.2.3). M ode-5 baseline risks for A tlas and D elta were recomputed using newly derived values for (1) shaping constants A and B, (2) the overall vehicle failure probability, and (3) the relative probabilities of occurrence of the individual failure-response modes. Results were then compared with baseline risks computed in prior RTI studies. For A tlas, M ode-5 launch-area risks were reduced by a factor between 3 to 11, the exact value depending on the assumed breakup qa for the vehicle. For D elta, the reduction factor was between 4 and 75, with the exact value again depending on assumed breakup conditions. 9/10/96 78 RTI Appendix A. Failure Response Modes in Program DAMP In program D A M P, no attempt is made to model vehicle behavior for failure of specific systems and components. A list of such failures and possible behaviors for any vehicle would be extensive, and variations from vehicle to vehicle would complicate the modeling process, or make it almost impossible. Instead, failure responses are modeled in D A M P without regard to the specific failure that causes the response. There are only six possible response modes in D A M P, five for failures, and one to model the behavior of a normal vehicle. The six vehicle-response modes are described in layman's language as follows; technical descriptions are provided in Ref. [1]. Mode 1: Vehicle topples over or falls back on the launch point after a rise of, at most, a few feet. Propellants deflagrate or explode with some assumed TNT equivalency. Mode 2: Vehicle loses control at or shortly after liftoff, with all flight directions equally likely. D estruct is transmitted as soon as erratic flight is confirmed, usually no later than six to twelve seconds after launch. For each vehicle, a latest destruct time is established that is used in computing the maximum impact distance for pieces, given that a M ode-2 response has occurred. Mode 3: Vehicle fails to pitch-program normally, producing near-vertical flight while thrusting at normal levels. Vehicle may tumble rapidly out of control at any point during vertical flight resulting in spontaneous breakup, or may be destroyed when destruct criteria are violated. The mode is terminated by destruct action if the vehicle readies the so-called "straight-up" time without programming. This time varies with launch vehide and with mission, but usually occurs (at C ape C anaveral A ir Station) between 30 and 70 seconds after launch. Mode 4: Vehide flies within normal limits until some malfunction terminates thrust, causes spontaneous breakup, or results in destruct by flight-control personnel. Breakup may or may not be preceded by a rapid tumble while the vehide is still thrusting but, in any event, vehide debris and components impad near the intended flight line. Mode 5: Vehide may impad in any direction from the launch point within its range capability. A t any range, impacts are most likely to occur along the flight line, becoming less likely as the angular deviation from the flight line increases. A s the impad range increases, weighting is progressively increased to favor the downrange direction. In any fixed direction, the impad probability decreases as the impad range increases. Flight may terminate spontaneously due to complete loss of vehide stability or because of destrud action. Outside the launch area, any malfunction with the potential to cause a substantial deviation from the intended flight direction is dassified as a M ode-5 failure response. By definition, M ode-5 9/10/96 79 RTI responses begin- at vehicle pitch-over or programming for vertically-launched missiles, and at liftoff for those not launched vertically. Mode 6: U nlike impacts from response M odes 1 through 5, M ode-6 impacts result from normal flights and normal impacts of separated stages and components. Jettisoned components are assumed to be non-explosive. For each impacting stage or component, a mean point of impact and bivariate-normal impact dispersions in downrange and crossrange components are assumed. The impact dispersions include the effects of variations in vehicle performance, drag uncertainties, and winds. Of the five failure-response modes, only M ode 5 is modeled to allow for the possibility of failure of the flight termination system, since vehicles experiencing other failure responses tend to impact within the impact limit lines. In D A M P, risk computations for M odes 2 through 4 are based on the assumption that the flight termination system is successfully employed when required. Failure responses originally classified as M ode 2, 3, or 4 may be reclassified as M ode 5 if the flight termination system fails or subsequent vehicle performance does not conform with the original response-mode definition. Risks associated with vehicle failure responses accompanied by a failure of the flight termination system are assumed to be adequately modeled in D A M F by M ode 5. The five failure-response modes modeled in D A M P are sufficient to account for all anomalous impacts in the estimation of risks. H owever, some vehicle failures and anomalous behaviors have an effect on mission success without increasing risks to people and property on the ground. These behaviors have been assigned Mode NA (not applicable) in the response-mode column of the launch-history tables in A ppendix D . 9/10/96 80 RTI Appendix B. Shaping-C onstant E ffects on Mode-5 Impact Distributions The values chosen for shaping constants A and B that appear in the M ode-5 impact-density function [Eq. (3)] have a significant effect on the angular distribution of impacts about the launch point. This A ppendix shows the effects of A and B on (1) the ratio of impacts along the downrange line to any other radial through the launch point and (2) the percentages of impacts in various sectors relative to the downrange line. Following the procedures outlined in Section 9.7 of Reference [1], it is interesting to observe the effects of varying the constants A and B. This is done in terms of a so-called f-ratio, which is expressed in Ref. [1] as Eq. (9.19), and is repeated here: f - ratio =--------1- (7) R The ratio shows how much more likely impact is to occur along the flight line (where 0 = n) than along some other radial line that makes an angle 9 (9 = k - A = 2.5 A = 3.0 A = 3.5 A = 4.0 A = 2.5 A = 3.0 A = 3.5 A = 4.0 0 1.0 1.0 1.0 1.0 1.0 1.0 1.0 1.0 5 1.2 1.3 1.4 1.4 1.2 1.3 1.4 1.4 10 1.5 1.7 1.8 2.0 1.5 1.7 1.8 2.0 15 1.9 2.2 2.5 2.8 1.9 2.2 2.5 2.8 20 2.3 2.8 3.4 4.0 2.3 2.8 3.4 4.0 25 2.8 3.6 4.6 5.7 2.9 3.7 4.6 5.7 30 3.4 4.7 6.2 8.1 3.6 4.8 6.2 8.1 35 4.1 6.0 8.4 11.5 44 6.1 8.4 11.5 40 4.9 7.7 11.3 16.2 5.3 7.9 11.4 16.3 45 5.8 9.8 15.3 23.0 6.5 10.2 15.5 23.1 50 6.8 12.4 20.5 32.4 7.9 13.2 20.9 32.7 55 8.0 15.7 27.5 45.8 9.6 16.9 28.3 46.2 60 9.3 19.7 36.7 64.5 11.5 21.6 38.1 65.4 65 10.7 24.4 48.8 90.6 13.7 27.5 51.2 92.3 70 12.1 29.9 64.3 126.7 16.2 34.8 68.7 130.2 75 13.5 36.3 84.1 176.4 19.0 43.8 91.7 183.1 80 15.0 43.4 108.6 243.9 22.1 54.5 121.8 256.9 85 16.4 51.1 138.4 333.9 25.4 67.3 160.6 358.9 90 17.8 59.1 173.5 451.4 28.8 82.2 209.9 498.3 95 19.0 67.3 213.3 600.5 32.4 98.9 271.3 686.6 100 20.1 75.3 256.8 782.9 35.9 117.3 345.7 936.0 105 21.2 82.9 302.1 996.3 39.4 137.0 433.3 1258.3 110 22.1 89.8 347.2 1233.5 42.7 157.2 532.8 1662.1 115 22.9 96.0 390.2 1482.5 45.9 177.4 641.3 2148.4 120 23.5 101.4 429.4 1728.6 48.7 196.9 754.5 2707.0 125 24.1 106.0 463.6 1957.9 51.3 215.0 867.2 3315.0 130 24.6 109.9 492.6 2159.9 53.5 231.5 974.6 3939.0 135 25.0 113.0 516.4 2329.5 55.5 245.9 1072.3 4542.1 140 25.3 115.5 535.5 2466.0 57.2 258.3 1158.0 5092.0 145 25.6 117.6 550.4 2572.4 58.6 268.8 1230.3 5567.4 150 25.8 119.2 562.0 2653.1 59.9 277.4 1289.7 5959.9 155 26.0 120.5 570.8 2713.1 60.9 284.5 1337.3 6271.7 160 26.1 121.5 577.5 2757.1 61.7 290.1 1374.6 6512.1 165 26.3 122.2 582.5 2789.0 62.4 294.6 1403.5 6693.0 170 26.4 122.8 586.3 2812.0 63.0 298.2 1425.6 6826.7 175 26.4 123.3 589.1 2828.4 63.4 301.0 1442.3 6924.4 180 26.5 123.7 591.2 2840.1 63.8 303.2 1454.9 6994.9 9/10/96 83 RTI Table 35. Effect on f-Ratio of Varying M ode-5 C onstant B (A = 3) - Part 1 R —1 nm ____ R = 5 nm 180-0 B = 500 B = 1000 B=2000 B = 500 B = 1000 B = 2000o 1.0 1.0 1.0 1.0 1.0 1.0 5 1.3 1.3 1.2 1.3 1.3 1.3 10 1.6 1.6 1.5 1.7 1.7 1.7 15 2.1 2.0 1.9 2.2 2.2 2.1 20 2.7 2.5 2.3 2.8 2.8 2.7 25 3.4 3.1 2.7 3.6 3.6 3.4 30 4.2 3.7 3.1 4.7 4.5 4.3 35 5.2 4.5 3.6 6.0 5.8 5.4 40 6.4 5.3 4.1 7.7 7.3 6.6 45 7.7 6.2 4.5 9.8 9.2 8.1 50 9.2 7.0 5.0 12.4 11.4 9.8 55 10.8 7.9 5.3 15.7 14.1 11.7 60 12.4 8.7 5.7 19.7 17.1 13.7 65 14.1 9.5 6.0 24.4 20.6 15.8 70 15.8 10.2 6.2 29.9 24.3 17.8 75 17.3 10.8 6.4 36.3 28.5 19.9 80 18.7 11.3 6.6 43.4 32.5 21.8 85 20.0 11.7 6.7 51.1 36.5 23.5 90 21.1 12.1 6.8 59.1 40.4 25.0 95 22.0 12.3 6.9 67.3 44.1 26.3 100 22.8 12.6 7.0 75.3 47.3 27.5 105 23.4 12.7 7.0 82.9 50.2 28.4 110 23.9 12.9 7.1 89.8 52.7 29.1 115 24.3 13.0 7.1 96.0 54.7 29.7 120 24.6 13.1 7.1 101.4 56.4 30.2 125 24.9 13.2 7.1 106.0 57.8 30.6 130 25.1 13.2 7.1 109.9 58.9 30.9 135 25.3 13.3 7.2 113.0 59.8 31.2 140 25.4 13.3 7.2 115.5 60.5 31.3 145 25.5 13.3 7.2 117.6 61.1 31.5 150 25.5 13.3 7.2 119.2 61.5 31.6 155 25.6 13.3 7.2 120.5 61.8 31.7 160 25.6 13.4 7.2 121.5 62.1 31.8 165 25.7 13.4 7.2 122.2 62.3 31.8 170 25.7 13.4 7.2 122.8 62.4 31.8 175 25.7 13.4 7.2 123.3 62.6 31.9 180 25.7 13.4 7.2 123.7 62.6 31.9 9/10/96 84 RTI _____ Table 36. Effect on f-Ratio of Varying M ode-5 C onstant B (A = 3) - Part 2 R = 10 nm II R = 25nm 180-0 B=500 B = 1000 B = 2000 B = 500 B = 1000 B = 2000 0 1.0 1.0 1.0 1.0 1.0 1.0 5 1.3 1.3 1.3 1.3 1.3 1.3 10 1.7 1.7 1.7 1.7 1.7 1.7 15 2.2 2.2 2.2 2.2 2.2 2.2 20 2.8 2.8 2.8 2.8 2.8 2.8 25 3.7 3.6 3.6 3.7 3.7 3.6 30 4.7 4.7 4.5 4.8 4.8 4.7 35 6.1 6.0 5.8 6.2 6.1 6.0 40 7.9 7.7 7.3 8.0 7.9 7.8 45 10.2 9.8 9.2 10.4 10.2 9.9 50 13.0 12.4 11.4 13.4 13.2 12.7 55 16.7 15.7 14.1 17.3 16.9 16.1 60 21.2 19.7 17.1 22.3 21.6 20.3 65 26.9 24.4 20.6 28.7 27.5 25.3 70 33.9 29.9 24.3 36.8 34.8 31.3 75 42.3 36.3 28.3 47.0 43.8 38.5 80 52.3 43.4 32.5 59.7 54.5 46.6 85 63.9 51.1 36.5 75.4 67.3 55.5 90 77.1 59.1 40.4 94.5 82.2 65.2 95 91.7 67.3 44.1 117.4 98.9 75.3 100 107.3 75.3 47.3 144.4 117.3 85.5 105 123.5 82.9 50.2 175.4 137.0 95.4 110 139.7 89.8 52.7 210.1 157.2 104.7 115 155.4 96.0 54.7 247.9 177.4 113.3 120 170.1 101.4 56.4 287.7 196.9 120.9 125 183.5 106.0 57.8 328.3 215.0 127.5 130 195.3 109.9 58.9 368.2 231.5 133.1 135 205.5 113.0 59.8 406.3 245.9 137.7 140 214.1 115.5 60.5 441.4 258.3 141.5 145 221.2 117.6 61.1 472.8 268.8 144.6 150 227.0 119.2 61.5 500.3 277.4 147.1 155 231.7 120.5 61.8 523.6 284.5 149.0 160 235.4 121.5 62.1 543.2 290.1 150.5 165 238.4 122.2 62.3 559.3 294.6 151.7 170 240.7 122.8 62.4 572.3 298.2 152.7 175 242.5 123.3 62.6 582.7 301.0 153.4 180 244.0 123.7 62.6 591.0 303.2 154.0 9/10/96 85 RTI The f-ratios in Table 33 and Table 34 (also in'Table 35 and Table 36) have been plotted in Figure 32 for A = 3.0 and B = 1000. Reading from the 10-mile plot for 9 = 90°, it can be seen that a vehicle experiencing a M ode-5 response is about 60 times more likely to impact along the flight line than along the 90-degree radial. Essentially the same value (actually 59.1) appears in Table 34. Angular D eviation From D ownrange (deg) Figure 32. f-Ratios for Ranges from 1 to 25 M iles 9/10/96 86 RTI There are other ways to show how the value chosen for A affects the M ode-5 impact density function. For five values of A , the plots in Figure 33 show the percentages* of A tlas H A S impacts that lie between the flight line and any radial line through the launch point that makes an angle 0 with respect to the flight line. If A = 3.0, it can be seen that approximately 46% of all M ode-5 impacts lie between 0° and 20°. If A is 4.0, the percentage of impacts between 0° and 20° increases to about 64% . * The Mode-5 impact density function must be integrated numerically to arrive at the values plotted in Figure 33. Since the quantity R that appears in the density function is trajectory dependent, somewhat different curves would be obtained for other trajectories and vehicles. Figure 33. Percentage of Impacts Between Flight Line and A ny Radial 9/10/96 87 RTI A nother way to show how the value of A affects M ode-5 impacts is illustrated in Figure 34. For the same values of A used previously in Figure 33, the graphs in Figure 34 show the percentages of impacts in any 5° sector between radials that make angles of 0° and (0 + 5)° with respect to the flight line. It is interesting to note that if A is set equal to 1.0 with B = 1,000, impacts in all 5° sectors are approximately the same, thus resulting in an impact-density function that is essentially uniform in direction. Angle from Flight Path, Theta (deg) Figure 34. Percentage of Impacts in 5-D egree Sectors For A = 1, the M ode-5 impact-density function is essentially the same as a density function formerly used in the Launch Risk A nalysis (LA RA ) Program at the W estern Range to model gross azimuth failures. This response mode was called the G ross Flight D eviation Failure (G FD F) mode. In LA RA the range and azimuth portions of the G FD F density function were assumed to be independent. Impact azimuths were uniformly distributed, while the range density function can be represented as f(R) = P tb r (8) 9/10/96 88 RTI where p is the probability of occurrence of the G FD F mode, TB is the stage bum time, and R is the rate of change of the impact range. The function cannot be applied early in flight before programming when R is essentially zero. The range portion of the M ode-5 impact-density function used in D A M P reduces to essentially the same form. If Eq. (3) is integrated between the limits of zero and n, the conditional M ode-5 density function reduces to «R) = ‘ , (9) (T.-TJR where Tp is the programming time, and TB and R are as previously defined. To obtain absolute values, f(R) must of course be multiplied by the probability of occurrence of a M ode-5 failure response. A lthough the G FD F density function may be a suitable model for random-attitude failures occurring at or a few seconds after programming, the performance histories in A ppendix D indicate that such failures are no more likely to occur at programming than at any other time. Thus, there appears to be no need for including a G FD F mode per se in the risk calculations, since all random-attitude failures are accounted for by the M ode-5 density function. H owever, if for some obscure reason inclusion of a G FD F response mode is desired, two approaches are possible: (l)run the G FD F mode separately in D A M P (by using M ode-5 with A = 1) while zeroing out all other response modes; (2) modify D A M P to handle two separate M ode-5 density functions, each with its own values of A and B. Obviously approach (2) is much more involved and time consuming to implement. A lthough it may not be obvious, the probability of impact in any annular range interval obtained by integrating the M ode-5 density function between the interval boundaries is independent of the values assigned to A and B. If Eq. (3) is integrated between the angle limits of zero and n (and only for these limits), the A 's and B's cancel leaving the probability of impact between Rj and Rj as a function of impact range alone. W ith a change of variable, the probability of impacting between R, and R, becomes a simple function of time (see pages 84 and 85 of Ref. [1] for details). 9/10/96 89 RTI Appendix C . Filter C haracteristics Estimating launch-vehicle failure probabilities using empirical launch data is an uncertain process when the sample size is small and the data are obtained from an evolving system. One approach that may be used to estimate failure probabilities is to perform a least-squares fit to trial outcome values (0 = success, 1 = failure). For mature launch vehicles, failure probabilities have decreased markedly from their early experimental days. For new programs, empirical data may be scant or nonexistent. One decision that must be made involves the type of function to' fit to the data. The true nature of the failure-rate function may be unknown or extremely complex, or there may be insufficient data to estimate a complex function. The easiest calculation is made when a constant failure-rate function is assumed. H owever, available data appear to indicate that failure rates decrease as a program matures, at least up to a point. If it can be assumed that launch-vehicle failure probabilities decrease over time (i.e., as the number of launches increases), then some non-constant function (perhaps linear or exponential) can be chosen for the fit, or the data weighted as a function of time. In estimating A tlas reliability, G eneral D ynamics'6’ chose the latter option by adopting the D uane model. This model is based on the assumption that the mean number of launches between failures increases when causes of failure are corrected. A lthough this may be the case up to' a point, eventually reliability seems to level off at a fairly constant value. C onsequently, for mature programs RTI has chosen to fit the failure­ rate function to a constant. Such a fit can be based on simple least squares using a fixed-length sliding-window filter to allow for changes in the estimated value over time, or on a least squares fit with unequal weighting. If a constant function is fit to a set of data using least squares with equal weighting of data, the solution is given by the mean: __ in x = -Y Xi (10) C onsider the following example: Xj = 6 x2 = 5 *3 = 7 Then, X = 6 + 5 + 7 __18 = 6 (11) 3 3 Recursively, 9/10/96 90 RTI Xn = Xn-1(l-an) + xn(an) . (12) For the equally-weighted case, the recursive filter factor an = 1/n. U sing the same example, with Xo = 0, Xi = Xj = 6 X2 = x1+l(x2-Xi) = 6 + |(5-6) = 5.5 (13) X3 = X2+-(x3-X2) = 5.5 + -(7-5.5) = 6.0 3 3 In general terms, this recursive formulation of the least squares solution is called an expanding-memory filter, as opposed to a sliding-window or fixed-length filter. In an expanding-memory filter, the solution is always based on the entire data set. In the equally-weighted case, all data points have an equal influence on the solution, regardless of their locations in the sequence. It can be seen that in the limit as n becomes very large, an approaches zero. That is, each data point in the sequence is accorded a decreased weight due to the increased number of points being fit. If the data being fit should actually describe a constant, this is exactly what is desired. Normally, however, the function that the data should fit is unknown, and a constant function is used merely as an approximation to smooth or edit the data. W hat is desired is a recursive least squares fit that assigns a decreasing weight to data of increasing age, so the fit de-weights data points used in earlier recursions. In a fading-memory filter, the weighting factor decreases as time recedes into the past, so that the importance of any given datum will decrease as the age of the datum increases. A n example of such a filter is one in which each datum is weighted by its count or index number in the sequence: n _ Six, X. = ---- (14) i=l U sing the same numerical example as before, where x: = 6, x2 = 5, and x3 = 7, * = 164^7 = 37 = M 7 1+2+3 6 9/10/96 91 RTI For the recursive form of this filter, where each datum is weighted by its position in the chronological sequence, the recursive filter factor for the n* point is given by = = 2n = 2 n y. n(n+l) n + 1 i=l U sing Eq. (12), n = 1 I ax = 1 I Xi = xx = 6 --------;--------j„---------- ------------------------- n = 2 a2=± X2=6 + -(5-6) = 5.33 _____ L_L_3J_______ £___ 1___________ n = 3 I a3 = | | X3 = 5.33+1(7 -5.33) = 6.17 (16) (17) The "memory" (i.e., importance) of older data in this filter fades at a rate dictated by the filter. In this case, the 50th value is 50 times more important than the first, and the 100th value is twice as important as the 50th and 100 times more important than the first. The exponentially-weighted filter provides the analyst with more flexibility. This filter uses F* as a weighting factor, where the filter-control constant F is a value chosen between zero and one, and i is the "age-count" of the i* data point. For this filter, i = 0 now designates the current or latest data point, i = 1 designates the immediately preceding or next-to-last data point, etc., so the data points are indexed in reverse chronological order starting with zero. The weighted least-squares solution is (18) U sing F = 0.9 and the same example as before, - F^+F^+FX F’+F'+F2 ._ (.9)°(7) + (.9)1(5)+(.9)2(6) (.9)°+(.9)1+(.9)2 = 7+ <5 + 4.86 16.36 = 2.71 ” 2.71 “ The weighting of each data point for sample sizes up to 300 is shown in Figure 35 for values of F from 0.8 to 1.0. For F = 1, all points in the sample are weighted equally. For 9/10/96 92 RTI F = 0.8, only the most recent 25 or so data points contribute to the final result, since all older data points are essentially weighted out of the solution. Figure 35. Exponential W eights for Fading-M emory Filters For the exponentially-weighted fading-memory filter, it can be shown that the recursive filter factor used in Eq. (12) is = 1-F &n 1-Fn (20) Since 0 < F < 1, an in Eq. (20) does not approach zero as n approaches infinity (as the other two filters do), but instead approaches the value (1 - F). If F = 0, then an = 1 for all n, the filter has no memory at all, and the filtered value always equals the last measurement. In the limit as F approaches one, L'H ospital's rule can be applied to 9/10/96 93 RTI show that an approaches 1/n, the filter-factor value for the equally-weighted case, and the filter memory no longer fades. For values of F between zero' and one, the rate at which the filter memory fades decreases as F increases. The analyst can control the rate at which the filter memory fades by selecting an appropriate value of F. A s the number of points n increases, the value of an used in the recursive exponential­ filter equation decreases continuously as it asymptotically approaches 1 - F. For any given n, a larger an means more emphasis is placed on the current data point and less on previous points. That is, the larger the recursive filter factor an, the faster the filter memory fades. Filter factors for sample sizes up to' 300 points are shown in Figure 36 for six different filters. Early in the data-index count (n less than 30), the filter based on index-number weighting has the fastest fading memory, since for 30 data points or fewer the filter has the largest filter factors. A fter 160 points or so, the index-weighted filter fades at a slower rate than the exponential filter with F = 0.99. C onsequently, users of index-count-based fading filters frequently calculate a filter factor for some maximum value of n that is then applied to all subsequent data points as well. For example, if a maximum count of about 180 is used for n; this filter from that point on will behave similarly to the exponentially-fading filter with F = 0.99. Number of D ata Points in Sample Figure 36. Recursive Filter Factor for Last D ata Point 9/10/96 94 RTI The fading-memory recursive filter, defined by Eqs. (12) and (20), can be applied to launch test results to estimate failure probability. For this application the values to be filtered are the test outcomes, with 0 representing a successful launch, and 1 representing a failure or anomalous behavior. G iven a series of outcomes, the filtered result after each launch in the series represents the estimate of failure probability at that point. Filtered results for two filter-control constants are shown in Table 37 for a hypothetical series of ten launches for which all but the second and fourth flights were successful. ______________ Table 37. Filter A pplication for Failure Probability_________________ F = 0.98 F = 0.90 Index Outcome Filter factor, an Fail. Prob. Filter factor, an Fail. Prob. 1 0 1.0000 0.0 1.0000 0.0 2 1 0.5051 0.5051 0.5263 0.5263 3 0 0.3401 0.3333 0.3690 0.3321 4 1 0.2576 0.5051 0.2908 0.5263 5 0 0.2082 0.3999 0.2442 0.3978 6 0 0.1752 0.3299 0.2132 0.3129 7 0 0.1517 0.2798 0.1917 0.2529 8 0 0.1340 0.2423 0.1756 0.2085 9 0 0.1203 0.2132 0.1632 0.17451..io 0 0.1093 0.1899 0.1535 0.1477 In this example, estimated failure probabilities are shown for two values of the filter constant that force the filter to fade at two different rates. A fter ten launches the estimated failure probability using F = 0.98 is 0.1899. For the faster fading-memory filter (F = 0.90), the result is 0.1477. Both estimates are less than that obtained by equal weighting, since the two failures occurred early in the sequence. Note that after four launches (2 successes and 2 failures) both filtered estimates exceed 0.5, since one of the two failures occurred during the fourth flight. If the l's and O's used in the example to represent failures and successes were reversed, the same filter would provide estimates of probability of success. 9/10/96 95 RTI Appendix D. Launch and Performance Histories D .1 Basic D ata In support of the empirical approach to use post-test results to estimate future vehicle failure rates, the performance histories for A tlas, D elta, Titan, and Thor missiles/ vehicles were studied. Results are summarized in A ppendix D as follows: A ppendix D . 2: A tlas Launch and Performance H istory A ppendix D . 3: D elta Launch and Performance H istory A ppendix D . 4: Titan Launch and Performance H istory A ppendix D . 5: Thor Launch and Performance H istory The histories include all A tlas, D elta, and Titan launches from the Eastern and W estern Ranges prior to 1 September 1996. For Thor, only Eastern Range launches are included, since this summary was completed before it was decided not to use Thor results in predicting failure probabilities for D elta. The A tlas, Titan, and Thor summaries include both weapons systems tests and space flights, while the D elta summary includes only space flights. For each vehicle, each section of the appendix is divided into two parts: (1) A tabular summary listing all launches in chronological order by sequence number, a mission identifier, launch date, vehicle configuration, launch range, the failure-response mode to which any failure has been assigned, the flight phase in which the failure or anomalous behavior occurred, and a configuration flag (0 or 1) indicating whether the vehicle is sufficiently representative of current vehicles to be included in the data sample used to predict vehicle reliability. (2) A brief narrative - necessarily brief in most cases due to lack of information - describing the general nature of the failure or the behavior of the vehicle after failure, or the effects of the failure on flight parameters. D .1.1 D ataSources The vehicle performance summaries and histories were collected primarily from the following sources: (1) "Eastern Range Launches, 1950 -1994, C hronological Summary", 45th Space W ing H istory Office.171 (2) Extension to (1) updating-the launch summary through 30 D ecember 1995.181 (3) "Vandenberg A FB Launch Summary", H eadquarters 30th Space W ing, Office of H istory, Launch C hronology, 1958 -1995.1’1 9/10/96 96 RTI (4) "Spacelift Effective C apacity: Part 1 - Launch Vehicle Projected Success Rate A nalysis", D raft prepared by Booz*A llen & H amilton, Inc. 19 February 1992, prepared for A ir Force Space C ommand Launch Services Office.141 (5) Isakowitz, Steven J., (updated by Jeff Samella), International Reference Guide to Space Launch Systems, Second Edition, published and distributed by A IA A in 1995.tl0] (6) Smith, O. G ., "Launch Systems for M anned Spacecraft", D raft, July 23,1991.[nl (7) "C omparison of Orbit Parameters - Table 1", prepared by M cD onnell D ouglas Space Systems C ompany, D elta launches through 4 Nov 95. (8) M issiles/Space Vehicle Files, 45th Space W ing, W ing Safety, M ission Flight C ontrol and A nalysis (SEO), 1957 through 1995.1131 (9) M issile Launch Operations Logs, 30th Space W ing, copies provided via A C TA , Inc., (M r. James Baeker), 1963 through 1995.'14' (10) "Titan IV, A merica's Silent H ero", published by Lockheed M artin in Florida Today, 13Nov95.1151 (11) "A tlas Program Flight H istory" (through A pril 1965), G eneral D ynamics Report EM -1860,26 A pril 1965.[W I (12) Fenske, C . W ., "A tlas Flight Program Summary", Lockheed M artin, A pril 1995.1171 (13) Brater, Bob, "Launch H istory", Lockheed M artin FA X to RTI, M arch 13,1996.[181 (14) Several U SA F A ccident/Incident Reports for A tlas and Titan failures.1191 (15) Quintero, A ndrew H ., "Launch Failures from the Eastern Range Since 1975", A erospace memo, February 25,1996, provided to RTI by Bill Zelinsky.1201 (16) Set of "Titan Flight A nomaly/Failure Summary" since 1959, received from Lockheed M artin, A pril 4, 1996.1211 (17) C hang, I-Shih, "Space Launch Vehicle Failures (1984 - 1995)", A erospace Report No. TOR-96(8504)-2, January 1996.122’ There were numerous discrepancies in the source data, particularly with regard to launch date and vehicle configuration. Some sources apparently list launch dates in local time, others use G reenwich time, and in some cases the same source may use both with no indication of which is which. M ost of the launch dates shown in A ppendix D agree with those in the Eastern Range and W estern Range summaries published by the respective H istory offices. Since the dates on these summaries are not consistently local or G reenwich, neither are the dates listed in A ppendix D . A lthough launch dates are 9/10/96 97 RTI used to order the vehicle tests for filtering, whether the dates are inconsistently in local or G reenwich times is inconsequential. In most cases, the ordering is not affected by a one-day change in launch date. In rare cases where the order of two launches might be inadvertently reversed, the filtering calculations are unaffected if the interchanged flights are both failures or both successes. Even when this is not the case, the effect on the final results for samples greater than one-hundred is negligible. C onfiguration discrepancies also existed in the source data as, for example, the listing of the same A tlas vehicle as a IIA in one source and as a H A S in another. In rare cases, a launch may have been called a success in one document and a failure in another, with little or no data provided to make it clear whether the difference in classification was due to error or different success criteria. A lthough a considerable effort was made to eliminate errors and discrepancies in A ppendix D , there can be no assurance that the effort was 100% successful. D .1.2 Assignment of Failure-Response Modes In the tabular historical summaries in A ppendix D , the column labeled "Response M ode" refers to the failure-response modes in program D A M P. The numbers 1 through 5 in this column correlate with the failure-response modes described in A ppendix A . The letter "T" following either a "3" or "4" indicates that the vehicle executed a thrusting tumble before breakup or destruct. A n "NA " (i.e., not applicable) appearing in the column means that some anomalous behavior caused stages or components to impact outside their normal impact areas without necessarily failing the flight, or that the anomalous behavior resulted in an unplanned orbit that may or may not have interfered with mission objectives. If the response-mode column is blank, either the flight was a success, or there was no information in the data sources to indicate otherwise. In some cases where the data sources contained only sketchy or incomplete information, assignment of the response mode involved some speculation; M ostly, this situation arose in trying to decide between response modes 4 and 5 or between modes 4 and 4T or, in rare cases, what mode to assign when the vehicle response did not exactly fit any of the response-mode definitions. D .1.3 Assignment of Flight Phase The number shown in the "Flight Phase" column in the tabular summaries of A ppendix D indicates the phase of vehicle flight in which the failure or anomalous behavior occurred. D efinitions of flight phase are given in Table 38. The assigned numbers are arbitrary, but were chosen in a way that suggests the vehicle stage that failed or the stage that was thrusting when the failure occurred. 9/10/96 98 RTI _________Table 38. Flight-Phase D efinitions_______________________ Flight PhaseD escription 0 SRM auxiliary thrust phase 1 First-stage thrust phase if no auxiliary SRM 's carried, or First-stage thrust phase after SRM separation 1.5 A ttitude-control phase after first-stage thrust phase or between first and second-thrust phases 2 Second-stage thrust phase 2.5 A ttitude-control phase after second thrust phase or between second and third-thrust phases 3 Third-stage thrust phase, or third thrust phase if second stage is restartable 3.5 A ttitude-control phase after third thrust phase or between third and fourth thrust phases 4 Fourth thrust phase, or U pper stage/payload thrust phase 5 A ttitude control phase after Flight Phase 4, or orbital phase In some cases, two flight phases are listed opposite an entry, e.g., 2 and 5. This means that some failure or anomalous behavior occurred during the second-stage thrusting period that did not prevent the attainment of an orbit, but did result in an abnormal final orbit. Other somewhat arbitrary decisions were necessary in assigning a flight phase when an expended stage failed to separate, or an upper stage failed to ignite. If, for example, the first and second stages failed to separate, any of flight phase 1,1.5, or 2 could be assigned, depending on the exact cause of the failure. The detailed information needed to make the proper choice was sometimes lacking. Table 39 is provided to assist in understanding how flight phases were assigned for A tlas, D elta/Thor, and Titan vehicles. Table 39. FlightJhases by Launch Vehic Flight PhaseA tlas D elta/Thor Titan 0 C astor burn C astor/G EM burn SRM solo 1 A tlas booster First-stage burn Stage 1 1.5 Booster separation Vernier solo - Sep 1/2 Stage-1 separation 2 Sustainer Second-stage burn Stage 2 2.5 Vernier/A C S solo C oast between stg 2/3 Vernier solo 3 A gena/C entaur Third-stage burn TS/C entaur/IU S 3.5 C oast after stg 3 4 Second burn Second burn Second burn 5 Orbit Orbit Orbit ... II 9/10/96 99 RTI D .1.4 Representative Configurations The last column in the tables in' A ppendix D indicates whether the vehicle configuration is considered sufficiently similar to current and future vehicles for the test result to be included in the representative data sample used to- predict absolute reliability. A "1" in the column indicates that the test result is included, while a "0" indicates that it is excluded. There are likely to be differences of opinion about which past configurations are representative and which are not. In determining which to include, RTI has relied entirely on the Booz«A llen & H amilton report141 referred to earlier. W hen faced with the same problem, Booz»A llen established the following criteria for deciding whether past configurations were sufficiently similar to current configurations: (1) G enealogy: Is the current system a direct or indirect derivative of the historical configuration? (2) Operations: Is the current system operated in the same manner as the historical configurations (e.g., IC BM versus space-launch vehicle)? (3) C omposition: D oes the current system use the same types of elements (i.e., SRM s, upper stage, etc.)? Based on these criteria and other factors, Booz*A llen decided to use test results from flights of the following vehicle configurations to predict future success rates: A tlas: SLV-3 and later configurations to include SLV-3A , SLV-3C , SLV-3D , G , H , I, II, IIA , IIA S. (Excluded: A tlas A , B, C , LV-3A , 3B, 3C , D , E, F) Delta: 291X and later configurations to include 391X, 392X, 492X, 592X, 692X, 792X. Titan: Titan IIIC and later configurations to include IIIB, H ID , H IE, 34B, 34D , III/C T, IV, II-SLV. 9/10/96 100 RTI D .2 Atlas L aunch and Performance H istory A tlas space-launch vehicles, originally manufactured by G eneral D ynamics and currently by Lockheed M artin, derived from the A tlas IC BM series developed in the 1950s. The primary one-and-one-half-stage vehicle played a major role in early lunar exploration activities (the unmanned Ranger, Lunar Orbiter, and Surveyor programs), and planetary probes (M ariner and Pioneer). Table 40 shows a summary of A tlas configurations since the beginning of the program.1101 Table 40. Summary of A das Vehicle C onfigurations C onfiguration D escription A IC BM single-stage test vehicle B,C IC BM 1% -stage test vehicle D IC BM and later space-launch vehicle E,F First an IC BM (1960), then a reentry test vehicle (1964), then a space-launch vehicle (1968) LV-3A Same as D except A gena upper stage LV-3B Same as D except man-rated for Project M ercury SLV-3 Same as LV-3A except reliability improvements SLV-3A Same as SLV-3 except stretched 117 inches LV-3C Integrated with C entaur D upper stage SLV-3C Same as LV-3C except stretched 51 inches SLV-3D Same as SLV-3C except C entaur uprated to D -1A and A tlas electronics integrated with C entaur (no longer radio guided) G Same as SLV-3D but A tlas stretched 81 inches H Same as SLV-3D except with E/F avionics and no C entaur I Same as G except strengthened for 14-ft payload fairing, ring laser gyro added II Same as I except A tlas stretched 108 inches, engines uprated, hydrazine roll-control added, verniers deleted, C entaur stretched 36 inches IIA Same as II except C entaur RL-lOs engines uprated to 20K lbs thrust and 6.5 seconds Isp increase from extendible RL-10 nozzles H A S Same as IIA except 4 C astor IVA strap-on SRM s added A tlas A , B, and C were developmental IC BM s. A tlas D , E, and F configurations were deployed as operational IC BM s during the 1960s. D uring that time, some A tlas D s were modified as space-launch vehicles in the LV series: LV-3A , 3B, and 3C . The Standardized Launch Vehicle (SLV) series derived from a need to reduce lead times in transforming A tlas missiles to space-launch vehicles. The SLV series began with the SLV-3 vehicle, which used an A gena upper stage. The G and H vehicles evolved from the SLV series. Eventually the I, II, IIA , and H A S configurations were developed with the aim of also supporting commercial launches. 9/10/96 101 RTI A tlas vehicles are fueled by a mixture of liquid oxygen and kerosene (RP-1). The latest IIA S configuration also incorporates C astor IVA solid-rocket motors. The early A tlas core vehicle included a sustainer, verniers, and two booster engines, all ignited prior to liftoff. In the A tlas II, IIA , and IIA S vehicles, the vernier engines have been replaced by a hydrazine roll-control system. Of the four C astor SRBs on the IIA S, two are ground lit and two are air lit some 60 seconds later. A tlas vehicles are now typically integrated with the C entaur upper stage vehicle that is fueled with liquid oxygen and liquid hydrogen. Earlier flights used an A gena upper stage. The entire A tlas history through 1995 is depicted rather compactly in bar-graph form in Figure 37. The solid-block portion of each bar indicates the number of launches during the calendar year for which vehicle performance was entirely normal, in so far as could be determined. The clear white parts forming the tops of most bars show the number of launches that were either failures or flights where the launch vehicle experienced some sort of anomalous behavior. Every launch with an entry in the response mode column in Table 41 falls in this category. Such behavior did not necessarily prevent the attainment of some, or even all, mission objectives. Figure 37. A tlas Launch Summary 9/10/96 102 RTI D .2.1 Atlas L aunch H istory The data in Table 41 summarize the flight performance of all A tlas and A tlas-boosted space-vehicle launches since the program began in June 1957. A launch sequence number is provided in the first column, a mission ID and launch date in columns 2 and 3. The vehicle configuration or A tlas booster number is given in the fourth column, while the fifth column shows whether the launch took place from the Eastern or W estern Range. The last three columns in the table show, respectively, the response mode assigned by RTI to any failure or anomalous behavior that occurred, the flight phase in which it occurred, and whether the vehicle configuration is considered representative for the purposes of predicting future A tlas reliability. Launches through sequence number 532 were used in the filtering process to estimate failure rate. Table 4. A tlas Launch H istory_____________________________ No. Mission/ID L aunch D ate Vehicle Configuration Test Range Response Mode Flight Phase Rep. Conf. 1 Weapons System (WS) 06 /11/57 4A ER 4T 1 0 2 WS 09/25/57 6 A ER 4 1 0 3 WS 12/17/57 12A ER 0 4 WS 01/10/58 10A ER 0 5 WS 02/07/58 13A ER 4 1 0 6 WS 02/20/58 11A ER 4T 1 0 7 WS 04/05/58 15A ER 4 1 0 8 WS 06 /03/58 16 A ER 0 9 WS 07/19/58 3B ER 4T 1 0 10 WS 08/02/58 4B ER 0 11 WS 08/28/58 5B ER 4 2.5 0 12 WS 09/14/58 8B ER 4 2.5 0 13 WS 09/18/58 6 B ER 4 1 0 14 WS 11/17/58 9B ER 4 i 2 0 15 WS 11/28/58 12B ER 0 16 SCORE 12/18/58 10B L V-3A/AGENA ER 0 17 WS 12/23/58 3C ER 0 18 WS 01/15/59 13B ER 5 1 0 19 WS 01/27/59 4C ER 5 2 0 20 WS 02/04/59 11B ER 0 21 WS 02/20/59 5C ER 4 2 0 22 WS 03/18/59 7C ER 4 1 0 23 WS 04/14/59 3D ER 4 1 0 24 WS - 05/18/59 7D ER 4 1 0 25 WS 06 /06 /59 5D ER 4 2 0 26 WS 07/21/59 8C ER 0 27 WS 07/28/59 11D ER 0 28 WS 08/11/59 14D ER 0 29 WS 08/24/59 11C ER 0 30 MERCURY (test) 09/09/59 10D L V-3B ER 4 2 0 31 D ESERT H EAT 09/09/59 12D _____________________ WR 0 9/10/96 103 RTI No. Mission/ID L aunch D ate Vehicle Configuration Test Range Response Mode Flight Phase Rep. Conf. 32 WS 09/16 /59 17D ER 4 2.5 0 33 WS 10/06 /59 18D ER 0 34 WS 10/09/59 22D ER 0 35 WS 10/29/59 26 D ER 4 2.5 0 36 WS 11/04/59 28D ER NA 2 0 37 WS 11/24/59 15D ER NA 2.5 0 38 ABL E (PIONEER) 11/26 /59 20D LV-3A/AGENA ER 4 1 0 39 WS 12/08/59 31D ER 0 40 WS 12/18/59 40D ER 0 41 WS 01/06 /6 0 43D ER 0 42 WS 01/26 /6 0 44D ER 0 43 D UAL EXH AUST 01/26 /6 0 6 D WR 4 2&2.5 0 44 WS 02/11/6 0 49D ER 0 45 MID AS I 02/26 /6 0 29D LV-3A/AGENAA ER 4 2.5 0 46 WS 03/08/6 0 42D ER 4 2.5 0 47 WS 03/10/6 0 51D ER 1 1 0 48 WS 04/07/6 0 48D ER 1 1 0 49 Q UICK START 04/22/6 0 25D WR 0 50 L UCKY D RAGON 05/06 /6 0 23D 'WR 3 1 0 51 WS 05/20/6 0 56 D ER 0 52 MID AS II 05/24/6 0 45D LV-3A/AGENAA ER 0 53 WS 06 /11/6 0 54D ER 0 54 WS 06 /22/6 0 6 2D ER 4 2.5 0 55 WS 06 /27/6 0 27D ER 0 56 WS 07/02/6 0 6 0D ER 4 2 0 57 TIGER SKIN 07/22/6 0 74D WR 5 1 0 58 MERCURY 1 07/29/6 0 50D L V-3B ER 4 1 0 59 WS 08/09/6 0 32D ER 0 6 0 WS 08/12/6 0 6 6 D ER 0 6 1 GOL D EN J OURNEY 09/12/6 0 47D WR 4 2 0 6 2 WS 09/16 /6 0 76 D ER 0 6 3 WS 09/19/6 0 79D ER 0 6 4 ABL E 5 (PIONEER) 09/25/6 0 80D L V-3A/AGENA ER 4T 2.5 & 3 0 6 5 H IGH ARROW 09/29/6 0 33D WR 4 1 0 6 6 WS 10/11/6 0 3E ER 5 2 0 6 7 Gibson Girl 10/11/6 0 57D LV-3A/AGENAA WR NA 3&5 0 6 8 D IAMOND J UBIL EE 10/12/6 0 81D WR 4 1 0 6 9 WS 10/13/6 0 71D ER 0 70 WS 10/22/6 0 55D ER 0 71 WS 11/15/6 0 83D ER . 0 72 WS 11/29/6 0 4E ER 5 2 0 73 ABLE 5B (PIONEER) 12/15/6 0 91D L V-3A/AGENA ER 4 1 0 74 H OTSH OT 12/16 /6 0 99D WR 0 75 WS 01/23/6 1 90D ER 0 76 WS 01/24/6 1 8E ER 5 2 0 77 J awhawk J amboree 01/31/6 1 70D LV-3A/AGENAA WR NA 2 : 0 9/10/96 104 RTI No. Mission/ID L aunch D ate Vehicle Configuration Test Range Response Mode Flight Phase Rep. Conf. 78 MERCURY 2 02/21/6 1 6 7D L V-3B ER 0 79 WS 02/24/6 1 9E ER 0 80 WS 03/13/6 1 13E ER 4 2 0 81 WS 03/24/6 1 16 E ER 4 1.5 0 82 MERCURY 3 04/25/6 1 100D LV-3B ER 3 1 0 83 WS 05/12/6 1 12E ER 0 84 L ITTL E SATIN 05/24/6 1 95D WR 0 85 WS 05/26 /6 1 18E ER 0 86 SURE SH OT 06 /07/6 1 27E WR 4 1 0 87 WS 06 /22/6 1 17E ER 4 1 0 88 WS 07/06 /6 1 22E ER 0 89 Polar Orbit (Midas III) 07/12/6 1 97D , L V-3A/AGENA B WR 0 90 WS 07/3176 1 21E ER 0 91 WS 08/08/6 1 2F ER 0 92 NEW NICKEL I 08/22/6 1 101D WR 0 93 RANGER 1 08/23/6 1 111D LV-3A/AGENA ER NA 4 0 94 WS 09/08/6 1 26 E ER 4 2 0 95 First Motion (Samos III) 09/09/6 1 106 D L V-3A/AGENAB WR 1 1 0 96 MERCURY 4 09/13/6 1 88D L V-3B ER 0 I 97 WS . 10/02/6 1 25E ER 0 98 WS 10/05/6 1 30E ER 0 99 Big Town (Midas IV) 10/21/6 1 105D L V-3A/AGENAB WR NA 2 0 100 WS 11/10/6 1 32E ER 4T 1 0 101 RANGER 2 11/18/6 1 117D L V-3A/AGENA ER NA 4 0 102 WS 11/22/6 1 4F ER 0 103 Round Trip (Samos IV) 11/22/6 1 108D L V-3A/AGENAB WR 4T 2 0 104 MERCURY 5 11/29/6 1 93D L V-3B ER 0 105 BIG PUSH 11/29/6 1 53D WR 0 106 WS 12/01/6 1 35E ER 0 107 BIG CH IEF 12/07/6 1 82D WR 0 108 WS 12/12/6 1 5F ER 5 2 0 109 WS 12/19/6 1 36 E ER 0 110 WS 12/20/6 1 6 F ER 4T 2 0 111 Ocean Way (Samos V) 12/22/6 1 114D L V-3A/AGENAB WR NA 2 0 112 BLUE FIN 01/17/6 2 123D WR 0 113 BL UE MOSS 01/23/6 2 132D WR 0 114 RANGER 3 01/26 /6 2 121D L V-3A/AGENAB ER NA 2&5 0 115 WS 02/13/6 2 40E ER 0 116 BIG J OH N 02/16 /6 2 137D WR NA 1.5 0 117 MERCURY 6 02/20/6 2 109D , L V-3B ER 0 118 CH AIN SMOKER 02/21/6 2 52D WR 4 1 0 119 SIL VER SPUR 02/28/6 2 6 6 E WR 4T 1.5 & 2 0 120 L oose Tooth 03/07/6 2 112D , L V-3A/AGENAB WR 0 121 CURRY COMB 1 03/23/6 2 134D WR 0 122 WS 04/09/6 2 11F ER 1 1 0 123 Night H unt 04/09/6 2 110D L V-3A/AGENA B WR NA 1 0 9/10/96 105 RTI Mission/ID L aunch D ate Vehicle Configuration Test Range Response Mode Flight Phase Rep. Conf. 124 CURRY COMB II 04/11/6 2 129D WR 0 125 RANGER 4 04/23/6 2 133D , L V-3A/AGENA B ER 0 126 D ainty D oll 04/26 /6 2 118D , L V-3A/AGENA B WR 0 127 BLUE BAL L 04/27/6 2 140D WR 0 128 AC-1 (SUBORBITAL) 05/08/6 2 104D L V-3C/CENT. D ER 4 1 0 129 CANNONBALL FLYER 05/11/6 2 127D WR 0 130 MERCURY 7 05/24/6 2 107D , L V-3B ER 0 131 Rubber Gun 06 /17/6 2 115D ,L V-3A/AGENAB WR 4 3 0 132 AL L J AZZ 06 /26 /6 2 21D WR 0 133 L ONG L AD Y 07/12/6 2 141D WR 0 134 EXTRA BONUS 07/13/6 2 6 7E WR 4 2&2.5 0 135 Armored Car 07/18/6 2 120D .L V-3A/AGENAB WR 0 136 FIRST TRY 07/19/6 2 13D WR 0 137 MARINER 1 (VENUS) 07/22/6 2 145D L V-3A/AGENAB ER 5 2 0 138 H IS NIBS 08/01/6 2 15F WR 0 139 Air Scout 08/05/6 2 124D , L V-3A/AGENA B WR 0 140 PEG BOARD 08/09/6 2 8D WR 0 141 PEG BOARD II 08/09/6 2 87D WR 4 2.5 0 142 CRASH TRUCK 08/10/6 2 57F WR 5 1 0 143 WS 08/13/6 2 7? ER 0 144 MARINER 2 (VENUS) 08/27/6 2 179D L V-3A/AGENAB ER NA 2 0 II 145 WS 09/19/6 2 8F ER 0 146 BRIAR STREET 10/02/6 2 4D WR 4 2 0 147 MERCURY 8 10/03/6 2 113D .L V-3B ER 0 148 RANGER 5 10/18/6 2 215D L V-3A/AGENAB ER NA 5 0 149 WS 10/19/6 2 14F ER 150 CL OSED CIRCUITS 10/26 /6 2 159D WR 0 151 WS 11/07/6 2 16 F ER 0 152 After D eck 11/11/6 2 128D , L V-3A/AGENA B WR 0 153 ACTION TIME 11/14/6 2 13F WR 4 1 0 154 WS 12/05/6 2 21F ER 0 155 D EER PARK 12/12/6 2 16 1D WR 0 156 Bargain Counter 12/17/6 2 131D , L V-3A/AGENA B WR 4T 1 0 157 OAK TREE 12/18/6 2 6 4E WR 4T 1 0 158 FL Y H IGH 12/22/6 2 16 0D WR 4 2 0 159 BIG SUE 01/25/6 3 39D WR 4 1 0 16 0 FAINT CLICK 01/31/6 3 176 D WR 0 16 1 FLAG RACE 02/13/6 3 182D WR 0 16 2 PITCH PINE 02/28/6 3 188D WR 0 16 3 ABRES-1 03/01/6 3 134F ER 0 16 4 TALL TREE 3 . 03/09/6 3 102D WR 5 1 0 16 5 TALL TREE 2 03/11/6 3 6 4D . WR 0 16 6 TALL TREE 1 03/15/6 3 46 D WR 4T 2 0 16 7 TALL TREE 5 03/15/6 3 6 3F WR 0 16 8 L EAD ING ED GE 03/16 /6 3 193D WR 4T 2 0 16 9 KEND ALL GREEN 03/21/6 3 83F WR 4 2.5 0 9/10/96 106 RTI No. Mission/ID L aunch D ate Vehicle Configuration Test Range Response Mode Flight Phase Rep. I Conf. 170 TAL L TREE 4 03/23/6 3 52F WR 4 1 0 171 BL ACK BUCK 04/24/6 3 6 5E WR NA 2.5 0 172 ABRES-2 04/26 /6 3 135F ER 0 173 D amp Clay 05/09/6 3 119D , L V-3A/AGENAB WR 0 174 MERCURY 9 05/15/6 3 130D , L V-3B ER 0 175 D OCK H AND 06 /04/6 3 6 2E WR 0 176 H ARPOON GUN 06 /12/6 3 198D WR 0 177 Big Four 06 /12/6 3 139D , L V-3A/AGENA B WR 4T 1 0 178 GO BOY 07/03/6 3 6 9E WR 0 179 Fish Pool 07/12/6 3 201D , L V-3A/AGENA D WR 0 180 D amp D uck 07/18/6 3 75D , L V-3A/AGENA B WR 0 181 SILVER D OLL 07/26 /6 3 24E WR 4 2 0 182 BIG FL IGH T 07/30/6 3 70E WR 0 183 COOL WATER I 07/31/6 3 143D WR 0 184 PIPE D REAM 08/24/6 3 72E WR 0 185 COOL WATER II 08/28/6 3 142D WR 0 186 Fixed Fee 09/06 /6 3 212D , L V-3A/AGENA D WR 0 187 COOL WATER III 09/06 /6 3 6 3D WR 4 1 0 188 COOL WATER IV 09/11/6 3 84D WR 4T 2.5 0 189 FILTER TIP . 09/25/6 3 71E WR 4T 2 0 190 H OT RUM 10/03/6 3 45F WR 1 1 0 191 COOL WATER V 10/07/6 3 16 3D WR 4 1 0 192 VEL A 1 &2 10/16 /6 3 197D , L V-3A/AGENA D ER 0 193 H ay Bailer 10/25/6 3 224D .L V-3A/AGENAD WR 0 194 ABRES-3 10/28/6 3 136 F ER 4T 2 0 195 H ICKORY H OL LOW 11/04/6 3 232D WR 0 196 COOL WATER VI 11/13/6 3 158D WR 4 1 0 197 AC-2 11/27/6 3 126 D .L V-3C/CENTAURD ER 0 198 L ENS COVER 12/18/6 3 233D WR 0 199 Rest Easy 12/18/6 3 227D , L V-3A/AGENA D WR 0 200 D AY BOOK 12/18/6 3 109F ^ 0 201 RANGER 6 01/30/6 4 199D .L V-3A/AGENAB ER 0 202 BL UE BAY 02/12/6 4 48E WR 4 2 0 203 Upper Octane 02/25/6 4 285D , L V-3A/AGENA D WR 0 204 ABRES-4 02/25/6 4 5E ER 0 205 Ink Blotter 03/11/6 4 296 D , L V-3A/AGENA D WR 0 206 ABRES-5 04/01/6 4 137F ER 0 207 H IGH BALL 04/03/6 4 3F WR 1 1 0 208 PROJ ECT FIRE 04/14/6 4 26 3D , L V-3A/AGENA D ER 0 209 Anchor D an 04/23/6 4 351D , L V-3A/AGENA D WR 0 210 Big Fred 05/19/6 4 350D , L V-3A/AGENA D WR 0 211 IRON L UNG 06 /18/6 4 2430 WR 0 212 AC-3 06 /30/6 4 135D , L V-3C/CENT. D ER 4 3 0 213 Q uarter Round 07/06 /6 4 352D , L V-3A/AGENA D WR 0 214 VELA3&4 07/17/6 4 216 D , L V-3A/AGENA D ER 0 215 RANGER 7 07/28/6 4 250D , L V-3A/AGENA D ER 0 9/10/96 107 RTI No. Mission/ID L aunch D ate Vehicle Configuration Test Range Response Mode Flight Phase Rep. Conf. 216 KNOCK WOOD 07/29/6 4 248D WR 0 217 L ARGE CH ARGE 08/07/6 4 110F WR 0 218 Big Sickle 08/14/6 4 7101, SL V-3A/AGENA D WR 1 219 GAL LANT GAL 08/27/6 4 57E WR 4 2 0 220 BIG D EAL 08/31/6 4 36 F WR 0 221 OGO-1 09/04/6 4 195D .L V-3A/AGENAB ER 0 222 BUTTERFLY NET 09/15/6 4 245D WR 0 223 BUZZING BEE 09/22/6 4 247D WR 0 224 Slow Pace 09/23/6 4 7102.SLV-3/AGENAD WR 1 225 Busy L ine 10/08/6 4 7103.SLV-3/AGENAD WR 1 226 Boon D ecker 10/23/6 4 353D .L V-3A/AGENAD WR 0 227 MARINER 3 11/05/6 4 289D .L V-3A/AGENAD ER 4 4 0 228 MARINER 4 11/28/6 4 288D .L V-3A/AGENAD ER 0 229 BROOKTROUT 12/01/6 4 210D WR 0 I 230 OPERA GL ASS 12/04/6 4 300D WR 0 I 231 Battle Royal 12/04/6 4 7105.SLV-3/AGENAD WR 1 232 ACM 12/11/6 4 146 D , L V-3C/CENTAUR D ER 0 233 STEP OVER 12/22/6 4 111F WR 0 234 PILOT L IGH T 01/08/6 5 106 F WR 0 235 PENCIL SET • 01/12/6 5 16 6 D WR 0 236 Beaver's D am 01/21/6 5 172D /ABRES WR 4 2&3 0 237 Sand L ark 01/23/6 5 7106 , SL V-3/AGENA D WR 1 238 RANGER 8 02/17/6 5 196 D , L V-3A/AGENA B ER 0 239 D RAG BAR 02/27/6 5 211D WR 0 240 PORK BARREL 03/02/6 5 301D WR 0 241 AC-5 03/02/6 5 156 D , L V-3C/CENT. D ER 1 1 0 242 Ship Rail 03/12/6 5 7104.SLV-3/AGENAD WR 1 243 ANGEL CAMP 03/12/6 5 154D WR 0 244 RANGER 9 03/21/6 5 204D ,L V-3A/AGENAB ER 0 245 FRESH FROG 03/26 /6 5 297D WR 0 246 Air Pump 04/03/6 5 7401, SL V-3/AGENA D WR 1 247 FLIP SID E 04/06 /6 5 150D WR 0 248 D warf Tree 04/28/6 5 7107, SL V-3/AGENA D WR 1 249 PROJ ECT FIRE 05/22/6 5 26 4D , L V-3A/AGENA D ER 0 250 Bottom L and 05/27/6 5 7108, SL V-3/AGENA D WR 1 251 Tennis Match 05/27/6 5 6 8D /ABRES WR 4 1 0 252 OL D FOGEY 06 /03/6 5 177D WR 0 253 L EA RING 06 /08/6 5 299D WR 0 254 STOCK BOY 06 /10/6 5 302D WR 0 255 Worn Face 06 /25/6 5 7109, SLV-3/AGENA D WR 1 256 BL IND SPOT 07/01/6 5 59D WR 0 257 White Pine 07/12/6 5 7112, SLV-3/AGENAD WR 4&5 2&3 1 I 258 VEL A5&6 07/20/6 5 225D , L V-3A/AGENA D ER 0 259 Water Tower 08/03/6 5 7111.SLV-3/AGENAD WR 1 26 0 PIANO WIRE 08/04/6 5 183D WR 0 26 1 SEA TRAMP 08/05/6 5 147F_____________________ WR 0 9/10/96 108 RTI No. Mission/ID L aunch D ate Vehicle Configuration Test Range Response Mode Flight Phase Rep. Conf. 26 2 AC-6 08/11/6 5 151D .L V-3C/CENTAURD ER 0 26 3 TONTO RIM 08/26 /6 5 6 1D WR 0 26 4 WATER SNAKE 09/29/6 5 125D WR 0 26 5 L og Fog 09/30/6 5 7110, SL V-3/AGENAD WR 1 26 6 Seething City 10/05/6 5 34D /ABRES WR 0 26 7 GTV-6 10/25/6 5 5301.SL V-3/AGENAD ER 4 3 1 26 8 Shop D egree 11/08/6 5 7113, SL V-3/AGENAD WR 1 26 9 WILD GOAT 11/29/6 5 200D WR 0 270 TAG D AY 12/20/6 5 85D WR 0 271 Blanket Party 01/19/6 6 7114.SL V-3/AGENAD WR 1 272 YEAST CAKE 02/10/6 6 305D WR 0 273 L ONEL Y MT. 02/11/6 6 86 D WR 0 274 Mucho Grande 02/15/6 6 7115, SL V-3/AGENAD WR 1 275 SYCAMORE RID GE 02/19/6 6 73D WR 0 276 ETERNAL CAMP 03/04/6 6 303D WR 5 1 0 277 GTV-8 03/16 /6 6 5302, SL V-3/AGENA D ER 1 278 D umb D ora 03/18/6 6 7116 , SL V-3/AGENAD WR 1 279 WH ITE BEAR 03/19/6 6 304D WR 5 2 0 280 Bronze Bell 03/30/6 6 72D WR 0 281 AC-8 ■ 04/07/6 6 184D , L V-3C/CENT. D ER 4T 4 . 0 282 OAO-1 04/08/6 6 5001.SL V-3/AGENAD ER 0 283 Shallow Stream 04/19/6 6 7117, SLV-3/AGENAD WR 1 284 CRAB CL AW 05/03/6 6 208D WR 4T 1 0 285 SUPPLY ROOM 05/13/6 6 98D WR 0 286 Pump H andle 05/14/6 6 7118, SL V-3/AGENAD WR 1 287 GTV-9 05/17/6 6 5303, SL V-3/AGENA D ER 5 1 1 288 SAND SH ARK 05/26 /6 6 41D WR 0 289 SURVEYOR-1 (AC-10) 05/30/6 6 290D , L V-3C/CENTAUR D ER 0 290 GTV-9A 06 /01/6 6 5304, SLV-3/AGENA D ER 1 291 Power D rill 06 /03/6 6 7119, SL V-3/AGENAD WR 1 292 OGO-3 06 /06 /6 6 56 01, SLV-3/AGENA B ER 1 293 Mama's Boy 06 /09/6 6 7201, SLV-3/AGENA D WR 1 294 VENEER PANEL 06 /10/6 6 96 D WR 4 2.5 0 295 GOLD EN MT. 06 /26 /6 6 147D WR 0 296 H EAVY ARTILL ERY 06 /30/6 6 298D WR 0 297 Snake Creek 07/12/6 6 7120, SL V-3/AGENA D WR 1 298 Stony Island 07/13/6 6 58D /ABRES WR NA 3 0 299 GTV-10 07/18/6 6 5305, SL V-3/AGENA D ER 1 300 BUSY RAMROD 08/08/6 6 149F WR 4 2 0 301 L UNAR ORBITER 1 08/10/6 6 5801.SL V-3/AGENAD ER 1 302 Silver D oll 08/16 /6 6 7121,SLV-3/AGENAD WR 1 303 H appy Mt. 08/19/6 6 7202, SL V-3/AGENA D WR 1 304 GTV-11 09/12/6 6 5306 , SL V-3/AGENA D ER 1 305 Taxi D river 09/16 /6 6 7123, SL V-3/AGENA D WR 1 306 SURVEYOR 2 (AC-7) 09/20/6 6 194D , L V-3C/CENT. D ER NA 5 0 307 D warf Killer 10/05/6 6 7203, SL V-3/AGENA D WR 1 9/10/96 109 RTI No. Mission/ID L aunch D ate Vehicle Configuration Test Range Response Mode Flight Phase Rep. Conf. 308 L OW H ILL 10/11/6 6 115F WR 4 1 0 309 Gleaming Star 10/12/6 6 7122, SL V-3/AGENAD WR 1 310 AC-9 10/26 /6 6 174D , L V-3C/CENT. D ER NA 2 0 311 Red Caboose 11/02/6 6 7124, SL V-3/AGENAD WR 1 312 L UNAR ORBITER 2 11/06 /6 6 5802, SL V-3/AGENAD ER 1 313 GTV-12 11/11/6 6 5307, SL V-3/AGENA D ER 1 314 Busy Mermaid 12/05/6 6 7125, SL V-3/AGENA D WR 1 315 ATS-B 12/06 /6 6 5101, SL V-3/AGENA D ER 1 316 Busy Panama 12/11/6 6 89D /ABRES WR 0 317 Busy Peacock 12/21/6 6 7001, SL V-3/AGENA D WR 1 318 BUSY STEPSON 01/17/6 7 148F WR NA 2.5 0 319 BUSY NIECE 01/22/6 7 35D WR 0 320 Busy Party 02/02/6 7 7126 , SL V-3/AGENAD WR 1 321 L UNAR ORBITER 3 02/04/6 7 5803, SL V-3/AGENAD ER 1 322 BUSY BOXER 02/13/6 7 121F 'WR 0 323 Giant Chief 03/05/6 7 7002, SL V-3/AGENA D WR 1 324 L ITTL E CH URCH 03/16 /6 7 151F WR 0 325 ATS-A 04/05/6 7 5102, SL V-3/AGENA D ER 1 326 BUSY SUNRISE 04/07/6 7 38D WR 0 327 SURVEYOR 3 (AC-12) 04/17/6 7 292D , L V-3C/CENTAUR D ER 0 328 Busy Tournament 04/19/6 7 7003, SL V-3/AGENA D WR 1 329 L UNAR ORBITER 4 05/04/6 7 5804, SL V-3/AGENA D ER 1 330 BUSY PIGSKIN 05/19/6 7 119F WR 0 331 Busy Camper 05/22/6 7 7127, SLV-3/AGENA D WR 1 332 Busy Wolf 06 /04/6 7 7128, SL V-3/AGENA D WR 1 333 BUCKTYPE 06 /09/6 7 122F WR 0 334 MARINER 5 (VENUS) 06 /14/6 7 5401, SL V-3/AGENA D ER 1 335 ABRES(AFSC) 07/06 /6 7 6 5D WR 0 336 SURVEYOR 4 (AC-11) 07/14/6 7 291D , L V-3C/CENTAUR D ER 0 337 ABRES(AFSC) 07122167 114F WR 0 338 AFSC 07127161 92D /ABRES WR 0 339 BREAD H OOK 07/28167 150F WR 0 340 L UNAR ORBITER 5 08/01/6 7 5805, SL V-3/AGENAD ER 1 341 SURVEYOR 5 (AC-13) 09/08/6 7 5901C, SLV-3/CENTAUR D ER 1 342 ABRES(AFSC) 10/11/6 7 6 9D WR 0 343 ABRES(AFSC) 10/14/6 7 118F WR 0 344 ABRES(AFSC) m/6781F WR 4T 1 0 345 ATS-C 11/05/6 7 5103,SLV-3/AGENAD ER 1 346 SURVEYOR 6 (AC-14) 11/07/6 7 5902C, SL V-3C/CENTAUR D ER 1 347 ABRES(AFSC) 11/07/6 7 94D WR 0 348 ABRES(AFSC) 11/10/6 7 113F WR 0 349 ABRES(AFSC) 12/21/6 7 117F WR 0 350 SURVEYOR 7 (AC-15) 01/07/6 8 5903C, SLV-3C/CENTAUR D ER 1 351 ABRES(AFSC) 01/31/6 8 94F WR 0 352 ABRES(AFSC) 02/26 /6 8 116 F WR 0 J 353 OGO-E 03/04/6 8 56 02A, SL V-3A/AGENA D ER ij 9/10/96 110 RTI No. Mission/ID L aunch D ate Vehicle Configuration Test Range Response Mode Flight Phase Rep. Conf. 354 ABRES(AFSC) 03/06 /6 8 74E WR 0 355 AFSC 04/06 /6 8 107F/ABRES WR 0 356 ABRES(AFSC) 04/18/6 8 77E WR 0 357 ABRES (AFSC) 04/27/6 8 78E WR 0 358 ABRES (AFSC) 05/03/6 8 95F WR 5 1 0 359 ABRES(AFSG) 06 /01/6 8 89F WR 0 36 0 ABRES(AFSG) 06 /22/6 8 86 F WR 0 36 1 ABRES(AFSC) 06 /29/6 8 32F WR 0 36 2 AFSC 07/11/6 8 75F/ABRES WR 0 36 3 D OD (AA-27) 08/06 /6 8 SLV-3A/AGENA D ER 1 36 4 ATS-D (AC-17) 08/10/6 8 5104C, SL V-3C/CENTAURD ER NA 4 1 36 5 AFSC 08/16 /6 8 7004.SLV-3/BURNER II WR 4 3 1 36 6 ABRES(AFSC) 09/25/6 8 99F WR 0 36 7 ABRES(AFSC) 09/27/6 8 84F WR 0 36 8 ABRES (AFSC) 11/16 /6 8 56 F WR 4T 2.5 0 36 9 ABRES (AFSC) 11^4/6 8 6 0F WR 0 370 OAO-A2 (AC-16 ) 12/07/6 8 5002C, SLV-3C/CENTAUR D ER 1 371 ABRES (AFSC) 01/16 /6 9 70F WR 0 372 MARINER 6 (MARS) (AC-20) 02/24/6 9 5403C, SLV-3C/CENTAUR D ER NA 1 1 373 AFSC ■ 03/17/6 9 104F/ABRES WR 0 374 MARINER 7 (MARS) (AC-19) 03/27/6 9 5105C, SL V-3C/CENTAUR D ER 1 375 D OD (AA-28) 04/12/6 9 SLV-3A/AGENAD ER 1 376 ATS-E (AC-18) 08/12/6 9 5402C, SL V-3C/CENTAUR D ER 1 377 ABRES (AFSC) 08/20/6 9 112F WR 0 378 ABRES (AFSC) 09/16 /6 9 100F WR 0 1 379 ABRES (AFSC) 10/10/6 9 98F WR 4 1 0 380 ABRES (AFSC) 12/03/6 9 44F WR 0 381 ABRES (AFSC) 12/12/6 9 93F WR 0 382 ABRES (AFSC) 02/08/70 96 F WR 0 383 ABRES (AFSC) 03/13/70 28F WR 0 384 ABRES (AFSC) 05/30/70 91F WR 0 385 ABRES (AFSC) 06 /09/70 92F WR 0 386 D OD (AA-29) 06 /19/70 SL V-3A/AGENAD ER 1 387 D OD (AA-30) 08/31/70 SLV-3A/AGENA D ER 1 388 OAO-B (AC-21) 11/30/70 5003C, SLV-3C/CENTAUR D ER 4 2 1 389 ABRES (AFSC) 12/22/70 105F WR 0 390 INTELSAT IV F-2 (AC-25) 01/25/71 5005C.SLV-3C/CENTAURD ER 1 391 ABRES (AFSC) 04/05/71 85F WR 0 392 MARINER 8 (MARS) (AC-24) 05/08/71 54050, SLV-3C/CENTAUR D ER 4T 3 1 393 MARINER 9 (MARS) (AC-23) 05/30/71 54040, SL V-3C/CENTAURD ER 1 394 ABRES (AFSC) 06 /29/71 103F WR 0 395 AFSC 08/06 /71 76 F WR 0 396 ABRES (AFSC) 09/01/71 74F WR 0 397 D OD (AA-31) 12/04/71 SL V-3A/AGENAD ER 4 1 1 398 INTEL SAT IV F-3 (AC-26 ) 12/19/71 5006 0, SLV-3C/CENTAUR D ER 1 399 INTEL SAT IV F-4 (AC-28) 01/22/72 50080, SLV-3C/CENTAUR D ER 1 9/10/96 111 RTI No. Mission/ID L aunch D ate Vehicle Configuration Test Range Response Mode Flight Phase Rep. Conf. 400 PIONEER 10 (AC-27) 03/02/72 5007C, SL V-3C/CENTAUR D ER 1 401 INTELSAT IV F-5 (AC-29) 06 /13/72 5009C, SL V-3C/CENTAUR D ER 1 402 OAO-C (AC-22) 08/21/72 5004C>SLV-3C/CENTAURD ER 1 403 AFSC 10/02/72 102F/BURNER II WR 0 404 D OD (AA-32) 12/20/72 SL V-3A/AGENA D ER 1 405 D OD (AA-33) 03/06 /73 SL V-3A/AGENAD ER 1 406 PIONEER 11 (AC-30) 04/05/73 5011D , SL V-3D /CENT D -1A ER 1 407 INTELSAT IV F-7 (AC-31) 08/23/73 5010D , SL V-3D /CENT D -1A ER 1 408 ABRES (AFSC) 08/29/73 78F WR 0 409 ACE 09/30/73 108F WR 0 410 MARINER 10 (AC-34) 11/03/73 5014D , SL V-3D /CENT D -1A ER 1 411 SFT-1 03/06 /74 73F WR 0 412 ACE 03/23/74 97F WR 0 413 SFT-2 05/01/74 54F WR 0 414 SFT-3 06 /28/74 82F WR 0 415 NTS-1 07/13/74 6 9F WR 0 416 ACE 09/08/74 80F WR 0 417 ABRES (AFSC) 10/1274 31F WR 0 418 INTELSAT IV F-8 (AC-32) 11/2174 5012D , SL V-3D /CENT D -1A ER 1 419 INTELSAT IV F-6 (AC-33) 02/2075 5015D , SL V-3D /CENT D -1A ER 4T 2 1 420 AFSC 04/1275 71F WR 4 1 0 421 INTELSAT IV F-1 (AC-35) 05/2275 5018D .SL V-3D /CENT D -1 A ER 1 422 D OD (AA-34) 06 /1875 SL V-3A/AGENA ER 1 423 INTELSAT IVA F-1 (AC-36 ) 09/2575 5016 D ,SL V-3D /CENTD -1A ER 1 424 INTELSAT IVA F-2 (AC-37) 01/2976 5017D , SL V-3D /CENT D -1A ER 1 425 AFSC 04/3076 F WR 0 426 COMSTAR D -1 (AC-38) 05/1376 5020D , SL V-3D /CENT D -1A ER 1 427 COMSTAR D -2 (AC-40) 07/2276 5022D , SL V-3D /CENTD -1A ER 1 428 D OD (AA-35) 05/2377 SL V-3A/AGENA ER 1 429 INTELSAT IVA F-4 (AC-39) 05/26 77 5019D , SL V-3D /CENT D -1A ER 1 430 NTS-2 06 /2377 6 5F WR 0 431 H EAO-A (AC-45) 08/1277 5025D , SL V-3D /CENT D -1A ER 1 432 INTELSAT IVA F-5 (AC-43) 09/2977 5701D , SL V-3D /CENT D -1 A ER 4T 1 1 433 AFSC 12/0877 F WR 0 434 D OD (AA-36 ) 12/1177 SL V-3A/AGENAD ER 1 435 INTELSAT IVA F-3 (AC-46 ) 01/06 78 5026 D , SL V-3D /CENT D -1A ER 436 FL TSATCOM-A (AC-44) 02/0978 5024D , SL V-3D /CENT D -1A ER 1 437 ND S-1 02/2278 6 4F WR 0 438 INTELSAT IVA F-6 (AC-48) 03/3178 5028D , SL V-3D /CENT D -1A ER 1 439 D OD (AA-37) 04/0778 SL V-3A/AGENA D ER 1 440 ND S-2 05/1378 49F WR 0 441 PIONEER (VENUS) (AC-50) 05/2078 5030D , SL V-3D /CENT D -1A ER 1 442 SEASATA 06 /26 78 23F/AGENA D WR 0 443 COMSTAR D -3 (AC-41) 06 /2978 5021D , SL V-3D /CENT D -1A ER 1 444 PIONEER (VENUS) (AC-51) 08/0878 5031D , SL V-3D /CENT D -1 A ER 1 L «J NAVSTAR III______________ 10/06 78 47F_____________________ WR 0 I 9/10/96 112 RTI No. Mlssion/ID L aunch D ate Vehicle Configuration Test Range Response Mode Flight Phase Rep. Conf. 446 TIROS N 10/13/78 29F WR 0 447 H EAO-B (AC-52) 11/13/78 5032D , SL V-3D /CENT D -1A ER 1 448 NAVSTARIV 12/10/78 39F WR 0 449 STP-78-1 02/24/79 27F WR 0 450 FL TSATCOM-B (AC-47) 05/04/79 5027D , SL V-3D /CENT D -1A ER 1 451 NOAA-A 06 /27/79 25F WR o 452 H EAO-C (AC-53) 09/20/79 5033D , SL V-3D /CENT D -1A ER 1 453 FL TSATCOM-C (AO49) 01/17/80 5029D , SL V-3D /CENT D -1A ER 1 454 NAVSTARV 02/09/80 35F WR 0 455 AFSC 03/03/80 F WR 0 456 NAVSTAR VI 04/26 /80 34F WR 0 457 NOAA-B 05/29/80 19F WR NA 1 0 458 FL TSATCOM-D (AC-57) 10/31/80 5037D , SLV-3D /CENTD -1A ER 1 459 INTELSAT IV F-2 (AC-54) 12/06 /80 5034D , SL V-3D /CENTD -1A ER 1 46 0 AFSC 12/08/80 6 8E WR 5 1 0 46 1 COMSTAR D (AC-42) 02/21/81 5023D , SL V-3D /CENTD -1A ER 1 46 2 INTELSAT V (AC-56 ) 05/23/81 5036 D .SL V-3D /CENTD -1A ER 1 46 3 NOAA-C 06 /23/81 87F WR 0 46 4 FL TSATCOM-E (AC-59) 08/06 /81 5039D , SL V-3D /CENT D -1A ER NA 1 &5 1 46 5 INTELSAT VF-3 (AC-55) 12/15/81 5035D , SL V-3D /CENTD -1A ER 1 46 6 NAVSTAR VII 12/18/81 76 E WR 2 1 0 46 7 INTELSAT VF-4 (AC-58) 03/05/82 5038D , SL V-3D /CENTD -1A ER 1 46 8 INTELSAT VF-5 (AC-6 0) 09/28/82 5040D , SL V-3D /CENT D -1A ER 1 46 9 D MSP F-6 12/20/82 6 0E WR 0 470 AFSC 02/09/83 H WR 1 471 NOAA-E 03/28/83 73E WR 0 472 INTEL SAT V F-6 (AC-6 1) 05/19/83 5041D , SLV-3D /CENTD -1A ER 1 473 AFSC 06 /09/83 H WR 1 474 NAVSTAR VIII 07/14/83 75E/PAM-D WR 0 475 D MSP F-7 11/17/83 58E WR 0 476 AFSC 02/05/84 H WR 1 477 INTELSAT VF-9 (AC-6 2) 06 /09/84 5042G/CENT D -1A ER 4T 4 1 478 NAVSTAR IX 06 /13/84 42E/PAM-D WR 0 479 NAVSTARX 09/08/84 14E/PAM-D WR 0 480 NOAA-F 12/12/84 39E WR 0 481 GEOSTA-A 03/12/85 41E WR 0 482 INTEL SATVF-10 (AC-6 3) 0322/85 5043G/CENT D -1A ER 1■ 483 INTELSAT VF-11 (AC-6 4) 06 /30/85 5044G/CENT D -1A ER 1 484 INTEL SATV F-12 (AC-6 5) 09/28/85 5045G/CENT D -1A ER 1 485 NAVSTAR XI 10/08/85 55E WR 0 486 AFSC 02/09/86 H WR 1 487 NOAA-G 09/17/86 52E WR 0 488 FLTSATCOM F-7 (AM6 ) 12/05/86 5046 G/CENT D -1A ER 1 489 FL TSATCOM F-6 (AC-6 7) 03/26 /87 5048G/CENTD -1A ER 4T 1 1 490 AFSC 05/15/87 H WR 1 491 D MSP F-8 06 /19/87 59E WR 0 9/10/96 113 RTI No. Misslon/ID L aunch D ate Vehicle Configuration Test Range Response Mode Flight Phase Rep. Conf. 492 D MSP F-9 02/02/88 54E WR 0 I 493 NOAA-H 09/24/88 6 3E WR 0 494 FL TSATCOM F-8 (AC-6 8) 09/25/89 5047G/CENT D -1A ER 1 495 P87-2 04/11/90 28E/AL T3A WR 0 496 CRRES (AC-6 9) 07/25/90 5049 l/CENT I ER 1 497 D MSS10 12/01/90 6 1E WR 0 498 BS-3H COMSAT (AC-70) 04/18/91 5050 l/CENT I ER 4T 3 1 499 NOAA-D 05/14/91 50E WR 0 500 D MSPF-11 11/28/91 53E WR 0 501 EUTEL SAT (AC-102) 12/07/91 8102II/CENTI ER 1 502 D SCS III (AC-101) 02/11/92 8101 ll/CENT I ER 1 503 GAL AXY 5 (AC-72) 03/14/92 5052 l/CENT ER 1 504 INTEL SAT K (AC-105) 06 /10/92 8105IIA/CENT ER 1 505 D SCS III (AC-103) 07/02/92 8103 ll/CENT ER 1 506 GALAXY 1R (AC-71) 08/22/92 5051 l/CENT ER 4T 3 1 507 UH F FOLL OW ON-1 (AC-74) 03/25/93 5054 l/CENT ER NA 2&5 1 508 D SCS III (AC-104) 07/19/93 8104 ll/CENT ER 1 509 NOAA-I 08/09/93 34E WR b 510 UH F F/O-2 (AC-75) 09/03/93 5055 l/CENT ER 1 511 D SCS III (AC-106 ) 11/28/93 8106 ll/CENT ER 1 512 TELSTAR4(AC-108) 12/16 /93 8201IIAS/CENT ER 1 513 GOES-1 (AC-73) 04/13/94 5053 l/CENT ER 1 514 UH F F/O-3 (AC-76 ) 06 /24/94 5056 l/CENT ER 1 515 D IRECT TV (AC-107) 08/03/94 8107 IIA/CENT ER 1 516 D MSPF-12 08/29/94 20E WR 0 517 INTELSAT VII (AC-111) 10/06 /94 8202 IIAS/CENT ER 1 518 ORION (AC-110) 11/29/94 8109 IIA/CENT ER 1 519 NOAA-J 12/30/94 11E WR 0 520 INTELSAT 704-2 (AC-113) 01/10/95 8203 IIAS/CENT ER 1 521 EH F F/O-4 (AC-112) 01/29/95 8110 ll/CENT ER 1 522 INTELSAT VII (AC-115) 03/22/95 8204 IIAS/CENT ER 1 523 D MSP F-13 03/24/95 45E WR 0 524 MSAT(AC-114) 04/07/95 8111 IIA/CENT ER 1 525 GOES-J (AC-77) 05/23/95 l/CENT ER 1 526 EH FF/O-5(AC-116 ) 05/31/95 ll/CENT ER 1 527 D SCS III (AC-118) 07/31/95 IIA/CENT ER 1 528 J CSAT (AC-117) 08/29/95 IIAS/CENT ER 1 529 EH F F/O-6 (AC-119) 10/22/95 ll/CENT ER 1 530 SOLAR OBSERV. (AC-121) 12/02/95 IIAS/CENT ER 1 531 GALAXY IIIR (AC-120) 12/15/95 IIA/CENT ER 1 I 532 PALAPA-C (AC-126 ) 01/31/96 . IIAS/CENT ER .1 533 INMARSAT-3 (AC-122) 04/03/96 IIA/CENT ER 1 534 SAX (AC-78) 04/30/96 l/CENT ER 1 535 UH F F7 (AC-125)__________ 07/25/96 ll/CENT ER 1 9/10/96 114 RTI D .2.2 Atlas Failure Narratives The following narratives provide the available details about each A tlas failure since the beginning of the A tlas program. The narratives are numbered to match the flight­ sequence numbers in Section D .2.1. 1. 4A , 11 June 57, Response M ode 4T, Flight Phase 1: Flight appeared normal for 24.7 seconds when drop in fuel supply to B2 engine produced a drop in performance and shutdown. Both engines moved to hardover in pitch to compensate for thrust asymmetry. The Bl engine failed at 27 seconds. A fuel fire was observed in aft end after thrust was lost. The missile continued to rise, reaching an altitude of 9,800 feet at 38 seconds. M issile was destroyed by safety officer 50.1 seconds after liftoff. Thrust unit and other hardware impacted about 1/4 mile south of launch pad (105° flight azimuth). 2. 6A , 25 Sep 57, Response M ode 4, Flight Phase 1: Flight appeared normal until about 32.5 seconds after liftoff, when performance level of both engines dropped to 35% of normal. Both engines shut down at 37 seconds. M issile was destroyed at 63 seconds. Loss of thrust was due to loss of LOX regulator in the booster gas generator. M ajor components impacted about 8000 feet downrange and 1000 feet right of flight line. 5. 13A , 7 Feb 58, Response M ode 4, Flight Phase 1: The B2 turbopump and engine stopped operating about 118 seconds due either to loss of LO 2 regulator reference pressure or a control-system failure. The Bl engine ceased to operate 0.3 second later. Failure was attributed to shorting of a vernier engine feedback transducer due to aerodynamic heating. Propellant sloshing that began building up at about 100 seconds led to missile instability. Vehicle broke up at 167 seconds. Impact occurred about 280 miles downrange and about 3 miles crossrange. 6. IIA , 20 Feb 58, Response M ode 4T, Flight Phase 1: Vernier engine was hardover from 51.9 seconds to 89.4 seconds, then returned to null until 104 seconds, then went hardover again. Other systems appeared normal until 109.6 seconds, when divergent oscillations began in rate-gyro outputs and engine positions. A ll engines reached stops by 114.3 seconds and continued thereafter to oscillate between stops until loss of thrust at 124.8 seconds. Vehicle breakup occurred one second later. Probable cause of oscillation was a component failure in flight control system. Vehicle impacted about 105 miles downrange and 8 miles right of flight line. 7. 15A , 5 A pr 58, Response M ode 4, Flight Phase 1: Booster engines shut down prematurely at 105.3 seconds (instead of planned 127 seconds) due to Bl turbopump failure. Since Bl chamber pressure drives the gas generator, the B2 turbopump and engine also stopped. Impact was 180 miles downrange and slightly left of flight line. 9/10/96 115 RTI 9. 3B, 19 July 58, Response M ode 4T, Flight Phase 1: Random failure of yaw rate gyro caused violent maneuvers resulting in rupture of LO 2 tank, engine shutdown, and a fire near the lube oil drain. M issile broke up about 42 seconds with impact about 2 miles downrange and 0.4 miles crossrange left. 11. 5B, 28 A ug 58, Response M ode 4, Flight Phase 2.5: M issile was normal to SEC O. A fter SEC O, failure of hydraulic system caused loss of vernier engine control. W arhead impacted close to intended target 12. 8B, 14 Sep 58, Response M ode 4, Flight Phase 2.5: W arhead impacted close to target although control was lost after SEC O due to failure of vernier-engine hydraulic system. 13. 6B, 18 Sep 58, Response M ode 4, Flight Phase 1: Except for a late-opening sustainer fuel valve, flight was apparently normal until 80.8 seconds, when the Bl turbopump failed. Performance of the Bl engine and the axial acceleration dropped sharply at about 81.7 seconds, and the B2 system shut down about 0.1 seconds later. The sustainer and vernier engines continued to operate normally until 82.9 seconds, when the missile exploded. Impact was about 25 miles downrange and about 0.6 miles right of the flight line. 14. 9B, 17 Nov 58, Response M ode 4, Flight Phase 2: The flight was terminated at 227.6 seconds by premature fuel depletion caused either by failure of the propulsion utilization system or by a tanking error. M issile impacted near the flight line about 2300 miles downrange, some 850 miles short of target. 18. 13B, 15 Jan 59, Response M ode 5, Flight Phase 1: The vehicle appeared normal for the first 50-60 seconds, at which time it was obscured by clouds. It was probably normal until about 100 seconds, but prelaunch removal of the mainframe telemetry system prevented a precise determination. Beginning about 101 seconds, various erratic pitch, yaw, and roll rates and oscillations were noted with accompanying drops in acceleration and velocity. These rates become excessive at 106.6 seconds. A t 121 seconds, the nosecone telemetry system showed that yaw and pitch rates abruptly increased, and this condition existed until reentry at 281 seconds. A ll thrusting apparently stopped between 121 and 123 seconds. The missile impacted about 170 miles downrange and 7.5 miles left. 19. 4C , 27 Jan 59, Response M ode 5, Flight Phase 2: Since the guidance system was inoperative throughout, the flight path was controlled by the pre-programmed flight control system. Impact was about 80 miles long and 30 miles left of target point. 21. 5C , 20 Feb 59, Response M ode 4, Flight Phase 2: A fter a normal booster phase, missile exploded at 173 seconds (BEC O at 149.2 sec) apparently due to loss of fuel­ tank pressure and subsequent rupture of LOX/fuel-tank bulkhead. Impact was about 1000 miles downrange and 6 miles left. 9/10/96 116 RTI 22. 7C , 18 M ar 59, Response M ode 4, Flight Phase 1: Booster engines shut down prematurely at 129.4 seconds, but booster section was not jettisoned until the near­ normal time of 153 seconds. G uidance was inoperative. Since the sustainer engine could not gimbal before booster separation, the autopilot was unable to stabilize the missile after BEC O. The sustainer shut down about 40 seconds before propellant depletion. The reentry vehicle spin rockets fired prematurely at 86.3 seconds after liftoff. 23. 3D , 14 A pr 59, Response M ode 4, Flight Phase 1: Performance of B2 engine dropped 36% at launch, resulting in a violent pitch as missile left the launcher. Flight control system corrected missile attitude, and flight continued at reduced thrust until a more violent explosion tore the thrust section away from the missile at 26.1 seconds. The sustainer continued operating with decreased thrust until shutdown by the safety officer at 36 seconds. D ebris impacted about 3000 feet from launch point. 24. 7D , 18 M ay 59, Response M ode 4, Flight Phase 1: Failure in pneumatic system resulted in missile explosion at 65 seconds. A temporary failure of the thrust­ structure fairing at liftoff strained the pneumatic lines and disconnects, resulting in leaks in the pneumatic system. 25. 5D , 6 June 59, Response M ode 4, Flight Phase 2: Either structural damage at booster staging or failure of the booster staging valve to close resulted in a fuel leak and explosion at 159.3 seconds. Impact occurred near the flight line about 780 miles downrange. 30. 10D (M ercury), 9 Sep 59, Response M ode 4, Flight Phase 2: Booster section failed to jettison resulting in a final velocity about 3000 ft/sec low and an impact range about 500 miles short of target. 32. 17D , 16 Sep. 59, Response M ode 4, Flight Phase 2.5: :Flight was considered a success since impact was within two miles of target point. H owever, failure of the vernier hydraulic package resulted in loss of missile control during the vernier solo phase. 35. 26D , 29 Oct 59, Response M ode 4, Flight Phase 2.5: Vernier solo phase was unstable in pitch due to loss of thrust from V2 vernier engine. The V2 engine lost chamber pressure during booster jettison. Impact was about 14 miles short and out of splash net. 36. 28D , 4 Nov 59, Response M ode NA , Flight Phase 2: The flight was normal, but was terminated prematurely when the range-safety impact-predictor system failed. 37. 15D , 24 Nov 59, Response M ode NA , Flight Phase 2.5: Flight was normal, except the reentry vehicle failed to arm or separate. 9/10/96 117 RTI 38. 20D (A ble IV), 26 Nov 59, Response M ode 4, Flight Phase 1: Third and fourth stages and payload broke off about 47 seconds. A tlas flight was normal and second stage ignited properly after A tlas SEC O. 43. 6D (D ual Exhaust), 26 Jan 60, Response M ode 4, Flight Phase 2 and 2.5: A t 175 seconds, as a result of a full-scale positive yaw command generated for five seconds, the missile stabilized on an erroneous heading. W hen a range-rate flag was lost 20 seconds later, the differentiated range-rate data substituted for measured data corrected the erroneous azimuth by generating a full-scale negative yaw command. The substituted data resulted in slightly erratic steering and a premature VEC O signal that was not acted upon. The verniers were subsequently cutoff by the backup signal. 45. 29D (M idas I), 26 Feb 60, Response M ode 4, Flight Phase 2.5: Flight was normal until firing of the retro rockets after A tlas separation. A n explosion at this time, probably due to activation of the A gena inadvertent separation destruct system, destroyed both the A tlas vehicle and the A gena. 46. 42D , 8 M ar 60, Response M ode 4, Flight Phase 2.5: Flight was considered a success although failure of the vernier hydraulic system resulted in loss of attitude control during the vernier solo phase. 47. 51 D , 10 M ar 60, Response M ode 1, Flight Phase 1: D ue to combustion instability, an explosion occurred in the Bl chamber before missile movement. M issile was destroyed at 2.5 seconds after 2-inch motion when main propellants ignited. 48. 48D , 7 A pr 60, Response M ode 1, Flight Phase 1: M issile was destroyed in launch stand during launch attempt, apparently due to combustion instability in the B2 thrust chamber. 50. 23D (Lucky D ragon), 6 M ay 60, Response M ode 3, Flight Phase 1: A n inoperative pitch gyro caused pitch instability, and resulted in destruct at 25.6 seconds. 54. 62D , 22 June 60, Response M ode 4, Flight Phase 2.5: Vernier engines were cutoff by autopilot backup when guidance discrete was not sent. Impact was 18 miles long. 56. 60D , 2 July 60, Response M ode 4, Flight Phase 2: D epletion of helium bottle pressure led to low sustainer and vernier engine thrust, and eventually early shutdown of engines. Impact was 40 miles short of target. 57. 74D (Tiger Skin), 22 July 60, Response M ode 5, Flight Phase 1: A pitchover rate that was 69% above the nominal rate resulted in vehicle breakup at 69.2 seconds. 9/10/96 118 RTI 58. 50D (M ercury), 29 July 60, Response M ode 4, Flight Phase 1: Flight appeared normal till 57.6 seconds when missile broke up apparently due to a rupture of the forward section of the LO 2 tank. 61. 47D (G olden Journey), 12 Sep 60, Response M ode 4, Flight Phase 2: Flight was apparently normal until about 222 seconds, when missile acceleration began to decay. A LOX regulator failure caused low sustainer performance and insufficient velocity to reach target. Impact was about 535 miles short. 64. 80D (A ble V/Pioneer), 25 Sep 60, Response M ode 4T, Flight Phase 2.5 and 3: A tlas performed normally except for failure of vernier engines to cut off. Flight was not successful since the A gena chamber pressure stabilized at 70% of normal shortly after ignition. Stage then apparently tumbled before cutting off 30 seconds early. Third-stage spun up and stabilized in a nose-down attitude. 65. 33D (H igh A rrow), 29 Sep 60, Response M ode 4, Flight Phase 1: The booster engines cut off prematurely and failed to separate from sustainer. The missile remained intact, but failed to achieve the desired range because of the added booster weight. 66. 3E, 11 Oct 60, Response M ode 5, Flight Phase 2: Sustainer hydraulic pressure began to decay at 41 seconds and dropped to zero at 62 seconds. Sustainer began tumbling at booster staging when control was essentially lost. Thrust continued for about 18 seconds moving the impact point some 270 miles farther downrange and 27 miles crossrange. The missile exploded at 155 seconds. 67. 57D (LV-3A )/A gena A (G ibson G irl), 11 Oct 60, Response M ode NA , Flight Phase 3 and 5: A tlas performance was satisfactory. A n umbilical failed to release properly from the A gena at liftoff, resulting in loss of pneumatic supply to the A gena attitude control system. A satisfactory orbit was not achieved. G uidance beacon failed at 106 seconds resulting in autopilot flight. 68. 81D (D iamond Jubilee), 12 Oct 60, Response M ode 4, Flight Phase 1: Overpressurization of the LOX tank resulted in tank rupture and vehicle breakup at 71.6 seconds. 72. 4E, 29 Nov 60, Response M ode 5, Flight Phase 2: Sustainer hydraulic pressure lost at 41 seconds. M issile tumbled shortly after booster staging. Sustainer thrust terminated at about 150 seconds, some 22 seconds after BEC O. D uring the sustainer solo phase, the impact point moved about 120 miles downrange and 44 miles crossrange. - 73. 91D , 15 D ec 60, Response M ode 4, Flight Phase 1: Vehicle performed normally till about 66.7 seconds, when a blast-band failure apparently resulted in rupture of the forward section of the LOX tank. The upper stages separated at this time, but the A tlas engines continued thrusting until 71 seconds. C ontrol was lost between 9/10/96 119 RTI 72 and 73 seconds, and a final explosion occurred at 74 seconds. Impact was about 8 miles downrange and one mile crossrange. 76. 8E, 24 Jan 61, Response M ode 5, Flight Phase 2: M issile stability was lost at about 161 seconds, some 30 seconds after BEC O, probably due to failure of the servo­ amplifier power supply. The sustainer engine shut down at 248 seconds, and the vernier engines about 10 seconds later. Impact occurred 1316 miles downrange and 215 miles crossrange. 77. 70D (LV-3A )/A gena A (Jawhawk Jamboree), 31 Jan 61, Response M ode NA , Flight Phase 2: Flight was considered successful although loss of rate lock at 222 seconds caused slightly erratic steering during the last 20 seconds of A tlas sustainer thrusting flight and failure of vehicle to pitch over during the vernier solo period. 80. 13E, 13 M ar 61, Response M ode 4, Flight Phase 2: Sustainer main fuel valve remained in the full open position throughout flight, resulting in fuel depletion and premature shutdown of sustainer engine at 251 seconds. 81. 16E, 24 M ar 61, Response M ode 4, Flight Phase 1.5: D ue to depletion of helium­ bottle pressure, booster section failed to jettison, leading to fuel depletion and impact far short of target. 82. 100D (M ercury 3), 25 A pr 61, Response M ode 3, Flight Phase 1: Flight was terminated at 40 seconds by RSO when vehicle failed to perform roll and pitch­ over maneuvers, apparently due to failure of the autopilot programmer. The malfunction was attributed to a plastic coating on the connector pins within the programmer, causing an open circuit. M ajor debris impacted about 1800 feet downrange and 6100 feet crossrange left. 86. 27E (Sure Shot), 7 June 61, Response M ode 4, Flight Phase 1: A pparent combustion instability caused an explosion and missile destruction 3.86 seconds after liftoff. 87. 17E, 22 June 61, Response M ode 4, Flight Phase 1: M issile destroyed itself at 101.5 seconds due to failure of flight-control system. Pitch rate was about 1.55 times normal. Just before breakup at 66,000 feet altitude, missile had pitched over almost 90° due to higher than normal pitch rate, producing excessive heating and aerodynamic loads. A t breakup, flight path was nearly horizontal. Impact was about 64 miles downrange. 93. lllD (Ranger-l), 23 A ug 61, Response M ode NA , Flight Phase 4: The A gena achieved a normal parking orbit. Flight continued normally until A gena second burn. D uring the restart sequence the fuel valve failed to open so only oxygen was pumped into the thrust chamber. A pogee of final orbit was only slightly above the normal circular parking-orbit altitude. 9/10/96 120 RTI 94. 26E, 8 Sep 61, Response M ode 4, Flight Phase 2: Sustainer engine shut down prematurely during the booster jettison sequence. M ost probable cause was drop in fuel flow to the gas generator. The vernier engines continued to burn for about 28 seconds after the sustainer shut down. Vernier thrust decayed at 137 seconds, guidance platform tumbled at 163 seconds. The missile remained intact until at least 470 seconds, when data were lost. Impact was about 525 miles downrange. 95. 106D (LV-3A )/A gena B (First M otion), 9 Sep 61, Response M ode 1, Flight Phase 1: Failure of an umbilical to eject allowed a commit/stop-power signal to reach the missile. Lack of electrical power 0.265 seconds after liftoff caused the vehicle to fall back on the launch pad after a rise of about 18 inches. 99. 105D (LV-3A )/A gena B (Big Town), M idas IV, 21 Oct 61, Response M ode NA , Flight Phase 2: Flight was regarded as a success, since the A gena compensated for A tlas anomalies. A tlas roll control was lost at 186 seconds, resulting in a roll rate of over 40° per second at A gena separation. C ontrol in pitch and yaw was maintained. A LOX leak affected sustainer performance just before SEC O and throughout the vernier phase. 100. 32E, 10 Nov 61, Response M ode 4T, Flight Phase 1: Sustainer engine shut down 0.7 seconds after liftoff. A lthough a fire appeared in the thrust section at 19 seconds, booster engines maintained stability until 24.5 seconds, when the B2 engine performance began to decay. A ll control was lost after this point, and the missile was destroyed by the RSO at 35 seconds. Impact was about 2500 feet downrange and 320 feet crossrange. 101. 117D (Ranger-2),18 Nov 61, Response M ode NA , Flight Phase 4: The A tlas booster functioned normally. A parking orbit was attained during the A gena first burn although roll control was not maintained due to failure of the roll gyro. W hen control gas was depleted, missile lost stability and began to tumble. Second A gena burn lasted only one second. 103. 108D (LV-3A )/A gena B (Round Trip), 22 Nov 61, Response M ode 4T, Flight Phase 2: Flight was not successful since vehicle failed to achieve orbit. Loss of pitch control at 244 seconds was attributed to aerodynamic heating. A t A gena separation the A tlas had pitched up 145°. 108. 5F,12 D ec 61, Response M ode 5, Flight Phase 2: A failure in the inertial guidance system of 1.06 seconds duration caused the existing inertial X velocity to be inserted in the Z-velocity channel. A s a result, the missile impacted 575 miles short and 30 miles left of target. 110. 6F, 20 D ec 61, Response M ode 4T, Flight Phase 2: Flight appeared normal until staging. D uring booster jettison, sustainer and vernier hydraulic pressure began to decay, leading to compete loss of sustainer yaw and pitch control at 229 and 232 seconds, respectively. M issile began tumbling at about 226 seconds. 9/10/96 121 RTI Sustainer engine shut down at 282 seconds. M issile impacted 1300 miles downrange and 18 miles crossrange. 111. 114D (LV-3A )/A gena B (Ocean W ay), 22 D ec 61, Response M ode NA , Flight Phase 2: Flight was considered successful although a failure in the flight programmer prevented the SEC O signal from cutting off the sustainer engine. Sustainer burned an additional 2.5 seconds to propellant depletion producing excess A tlas velocity. 114. 121 D (Ranger 3), 26 Jan 62, Response M ode NA , Flight Phase 2 and 5: Failure of pulse beacon in guidance system at 49 seconds caused sustainer to burn to LOX depletion, resulting in a 300 ft/sec overspeed. D ue to malfunction of pulse beacon at 49 seconds, no guidance steering commands or discretes were given. Booster was cut off by backup signal from accelerometer, sustainer by fuel depletion. D ue to excess speed, spacecraft passed 22,000 miles in front of moon, and primary mission objective was not met. A ll other A tlas and A gena systems performed as planned. 116. 137D (Big John), 16 Feb 62, Response M ode NA , Flight Phase 1.5: Flight was considered successful, although RV did not separate properly. 118. 52D (C hain Smoke), 21 Feb 62, Response M ode 4, Flight Phase 1: A fire in the engine compartment resulted in shutdown of all engines at 60 seconds and vehicle explosion at 72 seconds. 119. 66E (Silver Spur), 28 Feb 62, Response M ode 4T, Flight Phase 1.5 and 2: Loss of helium-bottle pressure resulted in failure to jettison booster engines and premature vernier-engine cutoff at 131.5 seconds. C utoff of verniers resulted in loss of roll control. Vehicle exploded at 295 seconds. 122. 11F, 9 A pr 62, Response M ode 1, Flight Phase 1: A n explosion in thrust section at 0.9 seconds after about 6 feet of motion was followed by a further explosion in the propellant tanks and total missile destruction at 1.2 seconds. 123. H OD (LV-3A )/A gena B (Night H unt), M idas, 9 A pr 62, Response M ode NA , Flight Phase 1: A n autopilot malfunction prevented sufficient pitchover during booster and sustainer phase resulting in improper SEC O conditions and an improper orbit. 128. 104D , 8 M ay 62, Response M ode 4, Flight Phase 1: Flight appeared normal until about 45 seconds when weather shield shifted. Further shocks occurred at 50 seconds with loss of weather shield. Booster-engine cutoff was initiated at 55 seconds. M issile destroyed itself at 57 seconds due to breakup of C entaur upper stage. Recorded impact was 8500 feet downrange and 8200 feet crossrange. 9/10/96 122 RTI 131. LV-3A /A gena B (Rubber G un), 17 June 62, Response M ode 4, Flight Phase 3: A lthough A tlas performance was satisfactory, the mission was apparently a failure. No other data available. 134. 67E (Extra Bonus), 13 July 62, Response M ode 4, Flight Phase 2 and 2.5: A LOX leak in the high-pressure line apparently froze sustainer control components. Residual sustainer thrust after cutoff continued for some 30 seconds, causing a 120-mile overshoot. 137. 145D (M ariner R-l), 22 July 62, Response M ode 5, Flight Phase 2: Booster stage and flight appeared normal until after booster staging at guidance enable at about 157 seconds. Operation of guidance rate beacon was intermittent. D ue to this and faulty guidance equations, erroneous guidance commands were given based on invalid rate data. Vehicle deviations became evident at 172 seconds and continued throughout flight with a maximum yaw deviation of 60° and pitch deviation of 28° occurring at 270 seconds. The vehicle deviated grossly from the planned trajectory in azimuth and velocity, and executed abnormal maneuvers in pitch and yaw. The missile was destroyed by the RSO at 293.5 seconds, some 12 seconds after SEC O. 141. 87D (Peg Board II), 9 A ug 62, Response M ode 4, Flight Phase 2.5: Failure of the sustainer/vernier hydraulic system to maintain system pressure prevented normal operation during the vernier solo phase. 142. 57F (C rash Truck), 10 A ug 62, Response M ode 5, Flight Phase 1: The roll program failed. The missile was destroyed by the RSO at 68 seconds. 144. 179D (M ariner R-2), 27 A ug 62, Response M ode NA , Flight Phase 2: Flight was successful although roll control was lost during the period from 140 seconds to 190 seconds due to erratic performance of vernier engine #2. Before and after this time interval, vernier #2 and all other A tlas and A gena systems performed normally. 146. 4D (Briar Street), 2 Oct 62, Response M ode 4, Flight Phase 2: The missile self­ destructed at 183 seconds. The vernier engines shut down prematurely at 46 seconds. Subsequently, closure of the vernier bleed valves led to excessively high sustainer performance and premature shutdown at 181.3 seconds. 148. 215 D (Ranger-5), 18 Oct 62, Response M ode NA , Flight Phase 5: Flight was regarded as successful although failure in the ground control system 35 minutes after launch prevented accomplishment of primary lunar impact and study mission. The guidance rate beacon failed at 94.6 seconds but backup differentiated tracking data kept the vehicle within normal limits. 153. 13F (A ction Time), 14 Nov 62, Response M ode 4, Flight Phase 1: The flight was terminated when sustainer and vernier engines shut down prematurely at 9/10/96 123 RTI 94.3 seconds. A thrust-section fire before 20 seconds apparently failed the lube oil system, which led to cessation of propellant flow. 156. 131D LV-3A /A gena B (Bargain C ounter), 17 D ec 62, Response M ode 4T, Flight Phase 1: M ission failed because of an A tlas hydraulic failure. M issile lost stability at 77.5 seconds, then rolled clockwise, pitched down and yawed left before breaking up at about 80.5 seconds. 157. 64E (Oak Tree), 18 D ec 62, Response M ode 4T, Flight Phase 1: The B2 engine failed at 37.1 seconds as a result of lubrication loss to the pinion gear. Booster engine shutdown resulted in a violent rolling yaw maneuver that caused missile breakup followed by an explosion at about 38 seconds. 158. 160D (Fly H igh), 22 D ec 62, Response M ode 4, Flight Phase 2: D ue to noisy data, range safety limits in the automatic cutoff system were exceeded, causing generation of an all-engines-cutoff signal. A s a result, the vernier engines were cut off about 10 seconds early, and the reentry vehicle was about 12.3 miles short. 159. 39D (Big Sue), 25 Jan 63, Response M ode 4, Flight Phase 1: Propulsion system performance was unsatisfactory after 78 seconds, when booster engine performance started to decay. Booster engines shut down' shortly after this, probably as a result of excessive heating in the gas-generator regulator. The sustainer operated normally until at least 106 seconds, with shutdown occurring sometime between 106 and 126 seconds. Breakup occurred about 300 seconds. M issile apparently impacted about 100 miles downrange. 164. 102D (Tall Tree 3), 9 M ar 63, Response M ode 5, Flight Phase 1: A flight-control malfunction occurred at about 15 seconds at the start of the pitch program. The missile pitched excessively, reaching 310° and an altitude of 5,000 feet at 33.5 seconds when it broke up. D ebris impacted close to pad. 166. 64D (Tall Tree 1), 15 M ar 63, Response M ode 4T, Flight Phase 2: A sustainer hydraulic-system failure at 83.5 seconds resulted in loss of sustainer engine control by 86 seconds and loss of vernier control at 99 seconds. M issile control was maintained by the booster engines until booster cutoff, when lack of sustainer and vernier control caused the missile to roll clockwise, pitch up, and yaw left. Sustainer thrust decayed at 131 seconds, and the missile began tumbling at 136.6 seconds. M issile self-destructed at 146 seconds with impact point about 600 miles downrange. 168. 193D (Leading Edge), 16 M ar 63, Response M ode 4T, Flight Phase 2: Loss of B2 pitch feedback signal at 103.5 seconds resulted in loss of vehicle stability. M issile tumbled, then self-destructed at about 270 seconds. 169. 83F (K endall G reen), 21 M ar 63, Response M ode 4, Flight Phase 2.5: A defective solder joint apparently led to two instances of erroneous velocity computations in 9/10/96 124 RTI the x and z velocity channels. A s a result, the missile impacted about 12 miles short and 0.2 miles right of target. 170. 52F (Tall Tree 4), 23 M ar 63, Response M ode 4, Flight Phase 1: M issile self­ destructed at about 91 seconds for unknown reasons. Impact was near the flight line about 120 miles downrange. 171. 65E (Black Buck), 24 A pr 63, Response M ode NA , Flight Phase 2.5: Vernier hydraulic-system pressure was lost at 301 seconds, resulting in loss of vernier­ engine control during the vernier solo phase. The reentry vehicle impact point was not perceptibly affected by this malfunction. 176. 139D LV-3A /A gena B (Big Four), 12 Jun 63: Response M ode 4T, Flight Phase 1: Flight appeared normal until about 88.4 seconds when, due to a hydraulic failure, the vehicle made a violent right and down maneuver. The missile broke up five seconds later at 93.4 seconds. 181. 24E (Silver D oll), 26 July 63, Response M ode 4, Flight Phase 2: Spurious voltage transients caused premature pressurization of the vernier solo tanks at 101.3 seconds, and premature sustainer engine shut down just after booster separation at 141 seconds. 187. 63D (C ool W ater III), 6 Sep 63, Response M ode 4, Flight Phase 1: A ll systems performed satisfactorily till 110 seconds, when the sustainer/vernier hydraulic pressure dropped from 3080 to 490 psig. The failure resulted in premature shutdown of the sustainer engine at 136 seconds. Booster-engine cutoff occurred normally at 140.3 seconds, and the booster was successfully jettisoned. The impact point occurred about 620 miles downrange. 188. 84D (C ool W ater IV), 11 Sep 63, Response M ode 4T, Flight Phase 2.5: Flight seemed normal through SEC O, although the pneumatic precharge to the vernier solo accumulator was lost at 96.6 seconds. D ue to this failure, missile stability was lost near the start of the vernier solo phase. The R/V probably failed to separate. 189. 71E (Filter Tip), 25 Sep 63, Response M ode 4T, Flight Phase 2: Visual observers reported a boat-tail fire, radical oscillations in yaw, and rough running booster and sustainer engines. Failure of the sustainer hydraulic system during the staging sequence resulted in loss of missile stability at 140 seconds. Sustainer and vernier engines shut down at about 267 seconds with the impact point about 600 miles downrange. 190. 45F (H ot Rum), 3 Oct 63, Response M ode 1, Flight Phase 1: The B-l booster-engine fuel valve failed to open during the start sequence, so the engine did not ignite. M issile toppled over and exploded. 9/10/96 125 RTI 191. 163D (C ool W ater V), 7 Oct 63, Response M ode 4, Flight Phase 1: Flight was normal up to about 73 seconds when the missile exploded. Suspected cause was intermediate bulkhead reversal/rupture due to insufficient helium pressure. 194. 136F (A BRES), 28 Oct 63, Response M ode 4T, Flight Phase 2: A fter a normal booster phase and staging, failure of sustainer hydraulic system resulted in loss of sustainer control and stability at 138 seconds. Sustainer and vernier engines shut down at 260 seconds, some 28 seconds early. The R/V impacted about 507 miles downrange. 196. 158D (C ool W ater VI), 13 Nov 63, Response M ode 4, Flight Phase 1: The trajectory was low throughout flight. The sustainer/vernier hydraulic pressure was lost at 112.7 seconds, followed by missile self-destruct at about 118 seconds when the vacuum impact point was about 280 miles downrange and on azimuth. 202. 48E (Blue Bay), 12 Feb 64, Response M ode 4, Flight Phase 2: The booster engine shut down at 119.5 seconds, and the sustainer engine shut down prematurely at 198.8 seconds. Impact was near the flight line about 635 miles downrange. 207. 3F (H igh Ball), 3 A pr 64, Response M ode 1, Flight Phase 1: M issile was destroyed on the pad when the Bl booster engine failed to ignite. 212. 135D (A C -3), 30 June 64, Response M ode 4, Flight Phase 3: The C entaur engines shut down early, apparently due to a hydraulic coupling failure that led to a failure in the propellant system. Impact was about 2340 miles downrange. 219. 57E (G allant G al), 27 A ug 64, Response M ode 4, Flight Phase 2: M issile experienced an early SEC O with no vernier burn thereafter due to a guidance­ system malfunction. Impact was about 88 miles short and 0.4 miles right of target. 227. 289D (M ariner-3),5 Nov 64, Response M ode 4, Flight Phase 4: A short second burn of the A gena prevented attainment of the desired orbit, and resulted in a heliocentric orbit. , 232. 146D , 11 D ec 64, Response M ode NA , Flight Phase 5: Flight was completely normal through C entaur first burn. D uring the coast phase, liquid hydrogen vented through the vent valve caused vehicle instability and tumbling. By second engine firing, insufficient liquid hydrogen remained at boost-pump' sump to sustain normal combustion. 236. 172D /A BRES (Beaver's D am), 21 Jan 65: Response M ode 4, Flight Phase 2 and 3: The A tlas apparently performed normally, except that the sustainer shut down 1.35 seconds early. The OV1-1 failed to-separate from the A tlas and thus failed to put the spacecraft in orbit. 9/10/96 126 RTI 240. 156D , 2 M ar 65, Response M ode 1 Flight Phase 1: A t 0.36 seconds booster fuel­ pump pressure dropped due to a fuel prevalve failure, booster lost thrust, fell back on launch pad, and was destroyed at 3.26 seconds. 251. 68D /A BRES (Tennis M atch), 27 M ay 65: Response M ode 4, Flight Phase 1: A failure in the booster gas-generator loop resulted in decreasing booster performance after 116 seconds. The impact point stopped moving at 122 seconds when an explosion occurred in the thrust section. Further vehicle breakup occurred at 218 seconds. D estruct was sent at 293 seconds. D ebris impacted close to the intended ground track. 257. SLV-3/A gena D (W hite Pine), 12 Jul 65: Response M ode 4 & 5, Flight Phase 2 & 3: Flight was normal until booster engines cutoff at 131 seconds. A s a result of a circuit board failure caused by excessive vibrations, the sustainer also shutdown at BEC O. The A tlas booster engines did not separate immediately from the sustainer, but did so some 50 seconds later after the event timer recycled. The A gena subsequently separated and ignited at about 198 seconds, creating wild uprange movements on the IP display by 255 seconds. D estruct was sent at 257 seconds. 267. SLV-3 (G TV-6), 25 Oct 65, Response M ode 4, Flight Phase 3: The flight was a failure although all A tlas objectives were achieved. The A gena startup appeared normal, but the engine shut down after about one second of operation, Propellants ceased flowing but the helium pressurization system continued to pressurize the propellant tanks until they burst. 276. 303D (Eternal C amp), 4 M ar 66, Response M ode 5, Flight Phase 1: A lthough track and rate lock were lost at 88 seconds, missile appeared normal till about 112 seconds when skyscreen operator reported that vehicle was spiraling. A hydraulic system failure occurred during the staging sequence, resulting in loss of vehicle stability at 153 seconds and sustainer engine shutdown at 194 seconds. The impact point initially appeared to stop about 800 miles downrange, well beyond the booster impact point. A t about this time or shortly thereafter, telemetry indicated rapidly varying pitch, roll, and yaw rates and shutdown of sustainer and vernier engines. Final impact was estimated to be 976 miles downrange and 3° left of the nominal track. 279. 304D (W hite Bear), 19 M ar 66, Response M ode 5, Flight Phase 2: The reentry vehicle impacted 82 miles beyond the target point when the head suppression valve failed to close at SEC O. The LOX tank thus vented through the sustainer chamber, adding impulse in the process. 281. 184D (A C -8) ,7 A pr 66, Response M ode 4T, Flight Phase 4: Flight appeared normal until second C entaur bum. Both C entaur engines started but one could not 9/10/96 127 RTI maintain thrust Thrust imbalance resulted in tumbling, followed by fuel starvation, and early thrust termination. 284. 208D (C rab C law), 3 M ay 66, Response M ode 4T, Flight Phase 1: H igh engine­ compartment temperatures were first noted at 41 seconds. The sustainer pitch­ actuator feedback-loop failed open at 136 seconds, a few seconds before planned BEC O. The flight appeared normal to the safety officer until about this time when roll and pitch rates increased. The IIP apparently stopped about 155 seconds, although G eneral D ynamics reported that vehicle stability was not lost until 216 seconds. Shutdown of sustainer and vernier engines occurred at 235 seconds. Suspected cause of malfunction was excessive heating in the boat-tail section. 287. SLV-3 (G TA -9), 17 M ay 66, Response M ode 5, Flight Phase 1: Vehicle became unstable when B2 pitch control was lost at 121 seconds. Loss of pitch control resulted in a pitch-down maneuver much greater than 90°. G uidance control was lost at 132 seconds. A fter BEC O, the vehicle stabilized in an abnormal attitude. A lthough the vehicle did not follow the planned trajectory, SEC O (at 280 seconds), VEC O (at 298 seconds), and A gena separation occurred normally from programmer commands. 294. 96D (Veneer Panel), 10 Jun 66, Response M ode 4, Flight Phase 2.5: The reentry vehicle undershot the target by 20 miles when the vernier engines shut down early. Failure was caused by an abnormal decay of control-bottle helium pressure. 298. 58D /A BRES (Stony Island), 13 July 66: Response M ode NA , Flight Phase 3: Flight was regarded as a success, although one of two OV's failed to orbit when it impacted the structure door which had not been opened. 300. 149F (Busy Ramrod), 8 A ug 66, Response M ode 4, Flight Phase 2: The sustainer engine shut down 27 seconds early due to' fuel depletion caused by an unfavorable ratio of propellant usage during the booster stage. Verniers burned to fuel depletion. 306. 194D (A C -7), 20 Sep 66, Response M ode NA , Flight Phase 5: A tlas C entaur performance was normal, but Surveyor spacecraft lost stability on the way to the moon. 308. 115F (Low H ill), 11 Oct 66, Response M ode 4, Flight Phase 1: The missile was normal till about 85 seconds when it appeared to lose thrust and breakup. Several major pieces impacted 32 to 40 miles downrange near the intended flight line. 310. 174D (A C -9), 26 Oct 66, Response M ode NA , Flight Phase 2: A lthough A tlas pressurization system anomaly caused decaying sustainer engine performance and early SEC O, no mission objectives were compromised. 9/10/96 128 RTI 318. 148F (Busy Stepson), 17 Jan 67, Response M ode NA , Flight Phase 2.5: Flight was normal except that reentry vehicle failed to separate. 344. 81F (A BRES/A FSC ), 27 Oct 67, Response M ode 4T, Flight Phase 1: A lthough various anomalous events occurred early in flight, the missile appeared to follow the intended trajectory till about 24 seconds. D iverging roll oscillations actually began about 21.4 seconds, and pitch and roll stability were lost by 24.8 seconds. By 27.9 seconds, the vehicle was tumbling about 6.5 degrees per second in pitch and yaw, and 12 degrees per second in roll. By 30 seconds, the vehicle lost all thrust and began to break up. Fuel cutoff and destruct were sent at 35 and 39 seconds, respectively. 358. 95F (A BRES/A FSC ), 3 M ay 68, Response M ode 5, Flight Phase 1: Immediately after liftoff the telemetered roll and yaw rates indicated that the missile was erratic. D uring the first 10 seconds of flight the missile yawed hard to the left. It then began a hard yaw to the right, crossed over the flight line and continued toward the right destruct line. Shortly thereafter the missile apparently pitched up violently and the IIP began moving back toward the beach. The missile was destructed at about 45 seconds when the altitude was about 14,000 feet and the downrange distance about 9 miles. M ajor pieces impacted less than a mile offshore, indicating uprange movement of the impact point during the last part of thrusting flight. 364. 5104C A C -17 (A TS-D ), 10 A ug 68, Response M ode NA , Flight Phase 4: A normal parking orbit was achieved, but when C entaur restart was attempted, thrust could not be maintained because of inoperative boost pumps. Frozen H 2O 2 line was the apparent root cause. 365. 7004 SLV-3/Bumer II/A gena D (A FSC ), 16 A ug 68: Response M ode 4, Flight Phase 3: A tlas performance was normal. The vehicle failed to achieve orbit because the protective shroud surrounding the second stage failed to separate. 368. 56F (A BRES/A FSC ), 16 Nov 68, Response M ode 4T, Flight Phase 2.5: Flight was normal through SEC O. The missile then lost attitude control, executing a hard yaw rate turn throughout and beyond the vernier solo phase. 372. 5403C A C -20 (M ariner 6 M are), 24 Feb 69, Response M ode NA , Flight Phase 1: Early A tlas BEC O due to staging accelerometer failure was compensated for by extended A tlas sustainer and C entaur burns. M ission was successful. 379. 98F (A BRES/A FSC ), 10 Oct 69, Response M ode 4, Flight Phase 1: The missile appeared normal until about 66 seconds when the sustainer engine shut down prematurely. The booster engine apparently continued normally to BEC O. A t about 255 seconds the payload SPD S engine ignited. D estruct was sent at 272 seconds. 9/10/96 129 RTI 388. 5003C A C -21 (OA O-B), 30 Nov 70, Response M ode 4, Flight Phase 2: Since the nose fairing failed to separate, C entaur did not have enough energy to make orbit. Payload impacted in A frica. 392. 5405C A C -24 (M ariner 8 M ars), 8 M ay 71, Response M ode 4T, Flight Phase 3: M ission requirements were not met. The A tlas boost phase was normal. Shortly after C entaur main-engine start, pitch stabilization was lost due to failure of the rate gyro or an electrical failure in the pitch channel of the flight control system. The vehicle began an accelerated nose-down tumbling motion that subsequently resulted in early and erratic main-engine shutdown due to propellant starvation. 397. SLV-3A (A gena), 4 D ec 71, Response M ode 4, Flight Phase 1: Sustainer engine turbine damage during engine start resulted in hot gas leaks and eventual failure of thrust-section hardware. Vehicle broke up at 87 seconds. 419. 5015D A C -33 (Intelsat IV F-6), 20 Feb 75, Response M ode 4T, Flight Phase 2: The A tlas booster-section electrical disconnect failed at booster staging. The harness was pulled apart, so flight-control avionics was unable to maintain vehicle stability: M issile appeared normal until the IP stopped at 200 seconds. Precautionary destruct was sent at 414 seconds. 420. 71F (A FSC ), 12 A pr 75: Response M ode 4, Flight Phase 1: A lthough an abnormal overpressure occurred at the base of the missile 620 msec before liftoff, the vehicle appeared normal until about 45 seconds when sustainer manifold and fuel-pump pressures began dropping. By 61 seconds, both the sustainer and vernier engines had shut down. Booster engines continued thrusting until about 123 seconds when the IIP stopped moving and radar operator reported multiple pieces. The breakup apparently resulted from an external explosion in the flame bucket that damaged the thrust section. D estruct was sent at 303 seconds when missile elevation dropped to 5°. 432. 5701D A C -43 (Intelsat IVA F-5), 29 Sep 77, Response M ode 4T, Flight Phase 1: A leak in the booster hot-gas generator at 2.3 seconds resulted in a fire in the thrust section at 36.5 seconds. The vehicle went into a violent maneuver at 54.9 seconds, failing the structure. The A tlas exploded at 55.8 seconds, leaving the C entaur intact. The C entaur was destroyed by the RSO at 61.7 seconds. 457. 19F (NOA A -B), 29 M ay 80: Response M ode NA , Flight Phase 1: Failure of turbopump seal allowed fuel to enter the gear box resulting in 21% low thrust by the Bl booster engine. The payload was inserted into an abnormal orbit and the mission was lost. 460. 68E, 8 D ec 80: Response M ode 5, Flight Phase 1: Flight appeared normal until 102.7 seconds when the lube oil pressure on the B2 booster engine suddenly dropped. A t 120.1 seconds, the engine shut down, followed 385 msec later by guidance shutdown of the Bl engine. The asymmetric thrust during shutdown 9/10/96 130 RTI caused yaw and roll rates that the flight control system could not correct. A s a result, attitude control was lost and the thrusting sustainer pivoted the missile to a retrofire attitude before the vehicle could be stabilized. A fter the booster package was jettisoned, the missile was stabilized and decelerating in the retrofire mode by 148 seconds. The sustainer continued thrusting in this attitude until 282.9 seconds when reentry heating apparently caused sustainer shutdown and vehicle breakup. 464. 5039D A C -59 (FLTSA TC OM ), 6 A ug 81, Response M ode NA , H ight Phase 1 and 5: The basic mission was accomplished although three increasingly severe shock events were recorded at 56.2, 70,7, and 120.8 seconds. The structural damage sustained by the spacecraft severely limited on-orbit operations. 466. 76E (NA VSTA R VII), 18 D ec 81: Response M ode 2, Flight Phase 1: Shortly after clearing the launch tower at an altitude of about two tower heights, the thrust performance of the Bl engine began to decay. The engine was shut down completely by 7.4 seconds. The unbalanced thrust caused the missile to pitch over to the right, and travel horizontally for about one second. It then pitched toward the ground. A small explosion occurred about one-third of the way down, followed by a larger explosion when the missile impacted the ground directly behind the launch pad about 19 seconds after liftoff. C ause of the engine failure was plugging of the gas-generator fuel-cooling parts that resulted in a gas­ generator bum-through. 477. 5042G A C -62 (Intelsat V), 9 Jun 84, Response M ode 4T, Flight Phase 4: Performance was normal until an abnormal shock event occurred at A tlas/C entaur separation. Subsequent data indicated that a C entaur oxygen tank leak resulted in a loss of 1483 pounds of LOX during C entaur first burn. The leak resulted in the LOX tank pressure falling below the LH 2 tank pressure, which led to collapse of the intermediate bulkhead during the coast phase. Bulkhead collapse caused unexpected tumbling forces during coast. The C entaur engines restarted after coast, but burned for only 6 or 7 seconds of a planned 90-second burn. 489. 5048G A C -67 (FLTSA TC OM F-6), 26 M ar 87, Response M ode 4T, FU ght Phase 1: Vehicle performance was normal till 48.4 seconds, when the vehicle was struck by lightning. A s a result, the guidance computer commanded a hard right turn which caused vehicle breakup due to inertial and aerodynamic loads. RSO sent destruct at 70.7 seconds. 498. 5050 A C -70 (BS-3H C OM SA T), 18 A pr 91, Response M ode 4T, Flight Phase 3: A tlas performance was normal. A lthough both C entaur main engines began the start sequence properly, the C -l turbo-machinery decelerated and stopped, leaving the C -l engine thrust at the ignition level. A ir entering through the stuck- open check valve liquefied and froze in the LH 2 pump and gear box of the C -l 9/10/96 131 RTI engine, thus preventing the engine from achieving full thrust. D ue to the resulting thrust imbalance, the vehicle tumbled out of control. D estruct was sent some 80 seconds after C entaur ignition. 506. 5051 A C -71 (G alaxy 1R), 22 A ug 92, Response M ode 4T, Flight Phase 3: A C entaur engine check valve stuck open allowing air into the turbopumps. A ir entering through the stuck-open check valve liquefied and froze in the LH 2 pump and gear box of the C -l engine, which prevented the engine from achieving full thrust. D estruct was sent by the RSO about 193 seconds after C entaur ignition. This is the same failure experienced by A C -70 launched on 18 A pr 91. 507. 5054 A C -74 (U H F Follow On-1), 25 M ar 93, Response M ode NA , Flight Phase 2 and 5: The flight was considered successful although below normal A das performance resulted in a low spacecraft apogee (5000 nm vice planned 9225 nm);' The perigee altitude was near nominal at 120 nm. A loose screw that allowed the oxygen regulator to go out of adjustment caused booster-engine thrust to drop to 65% of nominal at 103 seconds. The booster engines remained attached to the sustainer, which flew to propellant depletion. These events led to depletion shutdown of the C entaur stage 22 seconds early. 9/10/96 132 RTI D .3 D elta L aunch and Performance H istory The D elta launch-vehicle family originated in 1959 with a NA SA contract to D ouglas A ircraft C ompany, now M cD onnell D ouglas C orporation. The D elta, using components form U SA F's Thor IRBM program and U SN's Vanguard launch-vehicle program, was operational 18 months later. On M ay 13, 1960, the first D elta was launched from C ape C anaveral with a 179-pound Echo-I passive communications satellite. In the intervening years, the D elta has evolved to meet the ever-increasing demands of its payloads - including weather, scientific, and communications satellites. Each D elta modification corresponded to an increase in payload capacity. Table 42 shows a summary of D elta configurations since the beginning of the program.110’ The D elta 7925, the latest vehicle in the series, is a three-stage liquid-propellant vehicle with nine solid-propellant strap-on booster motors. For propellants, the D elta uses RP- 1 and liquid oxygen in Stage 1, and nitrogen tetroxide and aerozine 50 in Stage 2. Stage 3 consists of a Payload A ssist M odule (PA M ) with a solid-propellant motor. The strap-on boosters are H ercules graphite epoxy motors (G EM s) using H TPB-type solid propellant. A t liftoff, the liquid-propellant Stage-1 engine and six of the nine G EM s are ignited. The remaining three G EM s are ignited some 65 seconds later. Table 42. Summary of D elta Vehicle C onfigurations C onfiguration D escription D elta Stg. 1: M odified Thor. M B-3 Blk I engine Stg. 2: Vanguard A J10-118 propulsion system Stg. 3: Vanguard X-248 motor A Stg. 1: Engine replaced with M B-3 Blk II B Stg. 2: Tanks lengthened; higher energy oxidizer used C Stg. 3: Replaced with Scout X-258 motor PLF: Bulbous replaced low drag D Stg. 0: A dded 3 Thor-developed SRM s (C astor I) E Stg. 0: C astor II replaced C astor I Stg. 1: M B-3 Blk III replaced Blk II Stg. 2: Propellant tank diameters increased Stg. 3: Replaced with U SA F-developed FW -4 motor PLF: Fairing enlarged to 65-inch diameter J Stg. 3: TE-364-3 used L, M ,N Stg. 1: Tanks lengthened, RP-1 tank diameter increased Stg. 3: Varied: FW -4 (L), TE-364-3 (M ), none (N) M -6, N-6 Stg. 0: Six C astor Ils employed 900 Stg. 0: No C astor Ils employed Stg. 2: Replaced with Transtage A J10-118F engine 1604 Stg. 0: Six C astor Ils employed Stg. 3: Replaced with TE-364-4 9/10/96 133 RTI C onfiguration D escription 1910,1913, 1914 Stg. 0: Nine C astor Ils employed Stg. 3: Varied: none (1910), TE-364-3 (1913), TE-364-4 (1914) PLF: 96-inch diameter replaced 65-inch 2310,2313, 2314 Stg. 0: Three C astor Ils employed Stg. 1: RS-27 replaced M B-3 Stg. 2: TR-201 engine replaced A J10-118F Stg. 3: Varied: none (2310), TE-364-3 (2313), TE-364-4 (2314) 2910,2913, 2914 Stg. 0: Nine C astor Ils employed Stg. 3: Varied: none (2910), TE-364-3 (2913), TE-364-4 (2914) 3910,3913, 3914 Stg. 0: Nine C astor TVs replaced C astor Ils Stg. 3: Variedmone or PA M (3910),TE-364-3 (3913),TE-364-4 (3914) 3920,3924 Stg. 2: A J10-118K engine replaced TR-201 Stg. 3: Varied: none or PA M (3920), TE-364-4 (3924) 4920 Stg. 0: C astor IVA replaced C astor IV Stg. 1: M B-3 replaced RS-27 5920 Stg. 1: RS-27 replaced M B-3 6925 Stg. 1: Tanks lengthened 12 feet Stg. 3: STA R 48B motor used PLF: Bulbous 114-inch diameter used 7925 Stg. 0: G EM replaced C astor IVA Stg. 1: RS-27A replaced RS-27 9/10/96 134 RTI The entire D elta history through 1995 is depicted rather compactly in bar-graph form in Figure 38. The solid-block portion of each bar indicates the number of launches during the calendar year for which vehicle performance was entirely normal, in so far as could be determined. The clear white parts forming the tops of most bars show the number of launches that were either failures or flights where the launch vehicle experienced some sort of anomalous behavior. Every launch with an entry in the response-mode column in Table 43 falls in this category. Such behavior did not necessarily prevent the attainment of some, or even all, mission objectives. Figure 38. D elta Launch Summary 9/10/96 135 RTI D .3.1 D elta L aunch H istory The data in Table 43 summarizes all D elta and D elta-boosted space-vehicle launches since the program began. A launch sequence number is provided in the first column. A launch ID and date are provided in columns 2 and 3. The fourth column indicates the vehicle configuration. The fifth column indicates the launch range. The sixth column indicates the failure-response mode (1 through 5 and NA ) that RTI has determined best describes the failure that occurred. For M ode 3 or 4 failures, a suffix of 'T' indicates the vehicle tumbled. Successful launches are indicated by a blank in the Response-M ode column. The seventh column indicates the operational flight phase during which the failure occurred. The last column indicates whether the vehicle configuration is representative of those being launched today. Launches through sequence number 232 were used in the filtering process to estimate failure rate. Table 43. D elta Launch H istory No. Mission/ID L aunch D ate Vehicle Configuration Test Range Response Mode Flight Phase Rep. Conf. 1 ECH OI 05/13/6 0 D M-19 ER 4 2.5 0 2 ECH O IA 08/12/6 0 D M-19 ER 0 3 TIROS A2 11/23/6 0 D M-19 ER 0 4 P-14 03/25/6 1 D M-19 ER 0 5 TIROS A3 07/12/6 1 D M-19 ER 0 6 S-3 08/15/6 1 D M-19 ER 0 7 TIROS D 02/08/6 2 D M-19 ER 0 8 S-16 03/07/6 2 D M-19 ER 0 9 S-51 04/26 /6 2 D M-19 ER 0 10 TIROS E 06 /19/6 2 D M-19 ER NA 5 0 11 TSX-1 07/10/6 2 D M-19 ER 0 12 TIROS F 09/18/6 2 D M-19 ER 0 13 S-3A 10/02/6 2 D SV-3A ER 0 14 S-3B 10/27/6 2 D SV-3A ER 0 15 RELAYA-15 12/13/6 2 D SV-3B ER 0 16 SYNCOM A-25 02/13/6 3 D SV-3B ER 0 17 S-6 04/02/6 3 D SV-3B ER 0 18 TSX-2 05/07/6 3 D SV-3B ER 0 19 TIROS G 06 /19/6 3 D SV-3B ER 0 20 SYNCOM A-26 07/26 /6 3 D SV-3B ER 0 21 IMP A 11/26 /6 3 D SV-3C ER 0 22 TIROS H 12/21/6 3 D SV-3B ER 0 23 RELAYA-16 01/21/6 4 D SV-3B ER 0 24 S-6 6 03/19/6 4 D SV-3B ER 4 3 0 25 SYNCOM A-27 08/19/6 4 D SV-3D ER 0 26 IMP-B 10/03/6 4 D SV-3C ER NA 5 0 27 S-3C 12/21/6 4 D SV-3C ER 0 28 TIROS I 01/22/6 5 D SV-3C ER NA 2&5 0 29 OSO-B 02/03/6 5 D SV-3C ER 0 30 COMSAT #1 04/06 /6 5 D SV-3D ER 0 9/10/96 136 RTI No. Mission/ID L aunch D ate Vehicle Configuration fest Range Response Mode Flight Phase Rep. Conf. 31 IMP-C 05/29/6 5 D SV-3C ER 0 32 TIROS OT-1 07/01/6 5 D SV-3C ER 0 33 OSO-C 08/25/6 5 D SV-3C ER 4 2.5 0 34 GEOSA 11/06 /6 5 D SV-3E ER NA 2&5 0 35 PIONEER A 12/16 /6 5 D SV-3E ER 0 36 TIROS OT-3 02/03/6 6 D SV-3C ER 0 37 TIROS OT-2 02/28/6 6 D SV-3E ER 0 38 AE-B 05/25/6 6 D SV-3C ER NA 2&5 0 39 AIMP-D 07/01/6 6 D SV-3E ER NA 2.5 & 5 0 40 PIONEER-B 08/17/6 6 D SV-3E ER 0 41 TOS 10/02/6 6 D SV-3E WR 0 42 INTELSAT II (F-1) 10/26 /6 6 D SV-3E . ER 0 43 BIOS-A 12/14/6 6 D SV-3G ER 0 44 INTEL SAT II (F-2) 01/11/6 7 D SV-3E ER 0 45 TOS 01/26 /6 7 D SV-3E WR 0 46 OSO-E1 03/08/6 7 D SV-3C ER 0 47 INTELSAT II (F-3) 03/22/6 7 D SV-3E ER 0 48 TOSD 04/20/6 7 D SV-3E WR 0 49 IMP-F 05/24/6 7 D SV-3E WR 0 50 AIMP-E . 07/19/6 7 D SV-3E ER 0 51 BIOS-B 09/07/6 7 D SV-3G ER 0 52 INTEL SAT II (F-4) 09/27/6 7 D SV-3E ER 0 53 OSO-D 10/18/6 7 D SV-3C ER 0 54 TOS-C 11/10/6 7 D SV-3E WR 0 55 PIONEER-C 12/13/6 7 D SV-3E ER 0 56 GEOS-B 01/11/6 8 D SV-3E WR 0 57 RAE-A 07/04/6 8 D SV-3E WR 0 58 TOS-E 08/16 /6 8 D SV-3L WR 0 59 INTELSAT lll-A 09/18/6 8 D SV-3L ER 5 1 0 6 0 PIONEER-D 11/08/6 8 D SV-3E ER 0 6 1 H EOS-A 12/05/6 8 D SV-3E ER 0 6 2 TOS-F 12/15/6 8 D SV-3L WR r 0 6 3 INTEL SAT lll-C 12/18/6 8 D SV-3L ER 0 6 4 OSO-F 01/22/6 9 D SV-3C ER 0 6 5 ISIS-A 01/30/6 9 D SV-3E WR 0 6 6 INTEL SAT lll-B 02/05/6 9 D SV-3L ER 0 6 7 TOS-G 02/26 /6 9 D SV-3E ER 0 6 8 INTEL SAT lll-D 05/21/6 9 D SV-3L ER 0 6 9 IMP-G 06 /21/6 9 D SV-3E WR 0 70 BIOS-D 06 /29/6 9 D SV-3L ER 0 71 INTEL SAT lll-E 07/26 /6 9 D SV-3L ER 5 3&5 0 72 OSO-G 08/09/6 9 D SV-3L ER 0 73 PIONEER-E 08/27/6 9 D SV-3L ER 5 1 0 74 ID CSP/A-A 11/22/6 9 D SV-3L ER 0 I 75 INTEL SAT lll-F 01/14/70 D SV-3L ER 0 I 76 TIROS-M 01/23/70 D SV-3L__________________ WR L „q.. I 9/10/96 137 RTI No. Mission/ID L aunch D ate Vehide Configuration Test Range Response Mode Flight Phase Rep. Conf. 77 NATO-A 03/20/70 D SV-3L ER 0 79 INTELSAT lll-G 04/22/70 D SV-3L ER NA 1&5 o I 79 INTEL SAT lll-H 07/23/70 D SV-3L ER o I 80 ID CSP/A-B 08/19/70 D SV-3L ER o 81 ITOS-A 12/11/70 D SV-3L WR 0 82 NATO-B 02/03/71 D SV-3L ER 0 83 IMP-I 03/13/71 D SV-3L ER 0 84 ISIS-B 04/01/71 D SV-3E WR 0 85 OSO-H 09/29/71 D SV-3L ER NA 2&5 0 86 ITOS-B 10/21/71 D SV-3L WR 4 2 0 87 H EOS-A2 01/31/72 D SV-3L WR 0 I 88 TD -1 03/11/72 D SV-3L WR 0 89 ERTS-A 07/23/72 900 WR 0 90 IMP-H 09/22/72 16 04 ER 0 91 ITOS-D 10/15/72 300 WR 0 92 TELESAT-A 11/10/72 1914 ER o 93 NIMBUS-E 12/10/72 900 WR 0 94 TEL ESAT-B 04/20/73 1914 ER 0 95 RAE-B 06 /10/73 1913 ER 0 96 ITOS-E 07/16 /73 300 WR 4T 2 0 97 IMP-J 10/26 /73 16 04 ER 0 98 ITOS-F 11/06 ^3 300 WR 0 99 AE-C 12/16 /73 1900 WR 0 100 SKYNET IIA 01/19/74 2313 ER NA 4&5 0 101 WESTAR-A 04/13/74 2914 ER NA 1 1 102 SMS-A 05/17/74 2914 ER NA 1&5 1 103 WESTAR-B 10/10/74 2914 ER 1 104 ITOS-G 11/15/74 2310 WR 0 105 SKYNET-IIB 11/22/74 2313 ER 0 106 SYMPH ONIE-A 12/18/74 2914 ER 1 107 ERTS-B 01/22/75 2910 WR 1 108 SMS-B 02/06 /75 2914 ER 1 109 GEOS-C 04/09/75 1410 WR 0 110 TELESAT-C 05/07/75 2914 ER 1 111 NIMBUS-F 06 /12/75 2910 WR 1 112 OSO-I 06 /21/75 1910 ER 0 113 08/08/75 2913 WR 1 114 SYMPH ONIE-B 08/26 /75 2914 ER 1 115 AE-D 10/06 /75 2910 WR 1 116 GOES-A 10/16 /75 2914 ER 1 117 AE-E 11/19/75 2910 ER 1 118 RCA-SATCOM-A 12/12/75 3914 ER 1 119 CTS 01/17/76 2914 ER 1 120 MARISAT-A 02/19/76 2914 ER 1 121 RCA-SATCOM-B 03/26 /76 3914 ER 1 122 NATO-IH A 04/22/76 2914_______________ ER 1 9/10/96 138 RTI No. Mission/ID L aunch D ate Vehicle Configuration Test Range Response Mode Flight Phase Rep. Conf 123 L AGEOS 05/04/76 2913 WR 1 124 MARISAT-B 06 /10/76 2914 ER 1 125 PAL APA-A 07/08/76 2914 ER 1 126 ITOS-E2 07/29/76 2310 WR 0 127 MARISAT-C 10/14/76 2914 ER 1 128 NATOIIIB 01/27/77 2914 ER 1 129 PAL APA-B 03/10/77 2914 ER 1 130 ESRO-GEOS 04/20/77 2914 ER NA 2.5 & 5 1 131 GOES-B 06 /16 /77 2914 ER 1 132 GMS 07/14/77 2914 ER 1 133 SIRIO 08/25/77 2313 ER 0 134 OTS 09/13/77 3914 ER 4 1 1 135 ISEEA/B 10/22/77 2914 ER 1 136 METEOSAT-F1 11/22/77 2914 ER 1 137 CS 12/14/77 2914 ER 1 138 IUE 01/26 /78 2914 ER 1 139 L &SAT-C 03/05/78 2910 WR 1 140 BSE 04/07/78 2914 ER 1 141 OTS-2 05/11/78 3914 ER 1 142 GOES-C . 06 /19/78 2914 ER 1 143 ESRO-GEOS2 07/14/78 2914 ER 1 144 ISEE-C 08/12/78 2914 ER 1 145 NIMBUS-G 10/24/78 2910 WR 1 146 NATO IIIC 11/19/78 2914 ER 1 147 TELESAT-D 12/16 /78 3914 ER 1 148 SCATH A 01/30/79 2914 ER 1 149 WESTAR-C 08/09/79 2914 ER 1 150 RCA-C 12/07/79 3914 ER 1 151 SMM 02/14/80 3910 ER 1 152 GOES-D 09/09/80 3914 ER 1 153 SBS-A 11/15/80 3910 PAM ER 1 154 GOES-E 05/22/81 3914 ER 1 155 D E 08/03/81 3913 WR NA 2&5 1 156 SBS-B 09/24/81 3910 PAM ER 1 157 SME 10/06 /81 2310 WR 0 158 RCA-D 11/20/81 3910 PAM ER . 1 159 RCA-C' 01/15/82 3910 PAM ER 1 16 0 WESTAR-IV 02/26 /82 3910 PAM ER 1 16 1 INSAT-IA 04/10/82 3910 PAM ER 1 16 2 WESTAR-V 06 /09/82 3910 PAM ER NA 1 1 16 3 L &SAT-D 07/16 /82 3920 WR 1 16 4 TELESAT-F 08/26 /82 3920 PAM ER 1 16 5 RCA-E 10/27/82 3924 ER 1 16 6 IRAS 01/26 /83 3910 WR 1 16 7 RCA-F 04/11/83 3924 ER 1 16 8 GOES-F 04/28/83 3914_____________________ ER 1 9/10/96 139 RTI No. Mission/ID L aunch D ate Vehicle Configuration Test Range Response Mode Flight Phase Rep. Conf. 16 9 EXOSAT 05/26 /83 3914 WR 1 170 GALAXY-A 06 /28/83 3920 PAM ^ 1 171 TELSTAR-3A 07/28/83 3920 PAM ER 1 172 RCA-G 09/08/83 3924 ER 1 173 GALAXY-B 09/22/83 3920 PAM ER 1 174 L &SAT-D ' 03/01/84 3920 WR 1 175 AMPTE 08/16 /84 3924 ER 1 176 GAL AXY-C 09/21/84 3920 PAM ER 1 177 NATO-H ID 11/14/84 3914 ER 1 178 GOES-G 05/03/86 3914 ER 4 1 1 179 D EL TA 180 09/05/86 3920 ER 1 180 GOES-H 02/26 /87 3924 ER 1 181 PAL APA B2-P 03/20/87 3920 PAM ER 1 182 D EL TA 181 02/08/88 3910 ER 1 183 NAVSTAR11-1 02/14/89 6 925 ER 1 184 D EL TA STAR 03/24/89 3920 ER 1 185 NAVSTAR II-2 06 /10/89 6 925 ER 1 186 NAVSTAR II-3 08/18/89 6 925 ER 1 187 BSB-R1 08/27/89 4925 ER 1 188 NAVSTAR II-4 10/21/89 6 925 ER 1 189 OOBE 11/18/89 5920 WR 1 190 NAVSTAR II-5 12/11/89 6 925 ER 1 191 NAVSTAR II-6 01/24/90 6 925 ER 1 192 L OSAT 02/14/90 6 920-8 ER 1 193 NAVSTAR II-7 03/26 /90 6 925 ER 1 194 PAL APA B-2R 04/13/90 6 925 ER 1 195 ROSAT 06 /01/90 6 920-10 ER 1 196 INSAT-1 D 06 /11/90 4925 ER 1 197 NAVSTAR II-8 08/02/90 6 925 ER 1 198 BSB-R2 08/18/90 6 925 ER 1 199 NAVSTAR II-9 10/01/90 6 925 ER 1 200 INMARSAT-2F1 10/30/90 6 925 ER 1 201 NAVSTAR 11-10 11/26 /90 7925 ER 1 202 NATO IVA 01/07/91 7925 ER 1 203 INMARSAT-2F2 03/08/91 6 925 ER 1 204 ASC-2 04/12/91 7925 ER 1 205 AURORA II 05/29/91 7925 ER 1 206 NAVSTAR 11-11 07/03/91 7925 ER 1 207 NAVSTAR 11-12 02/23/92 7925 ER 1 208 NAVSTAR 11-13 04/09/92 7925 ER 1 209 PAL APA B4 05/13/92 7925-8 ER 1 210 EUVE 06 /07/92 6 920-10 ER 1 211 NAVSTAR 11-14 07/07/92 7925 ER 1 212 GEOTAIL 07/24/92 6 925 ER 1 213 SATCOM C4 08/31/92 7925 ER 1 214 NAVSTAR 11-15 09/09/92 7925 ER 1 9/10/96 140 RTI No. Mission/ID L aunch D ate Vehicle Configuration Test Range Response Mode Flight Phase Rep. Conf. 215 COPERNIKUS 10/12/92 7925 ER 1 216 NAVSTAR11-16 11/22/92 7925 ER 1 217 NAVSTAR11-17 12/18/92 7925 ER 1 218 NAVSTAR 11-18 02/03/93 7925 ER 1 219 NAVSTAR 11-19 03/30/93 7925 ER 1 220 NAVSTAR 11-20 05/13/93 7925 ER 1 221 NAVSTAR 11-21 06 /26 /93 7925 ER 1 222 NAVSTAR II-22 08/30/93 7925 ER 1 223 NAVSTAR II-23 10/26 /93 7925 ER 1 224 NATOIVB 12/08/93 7925 ER 1 225 GAL AXY l-R 02/19/94 7925-8 ER 1 226 NAVSTAR II-24 03/10/94 7925 ER 1 227 WIND 11/01/94 7925-10 ER 1 228 KOREASAT 08/05/95 7925 ER NA 1 &5 1 229 RAD AR SAT 11/04/95 7920-10 ER 1 230 X-RAY EXPLORER 12/30/95 7920A-10 ER 1 231 KOREASAT-2 01/14/96 7925 ER 1 232 NEAR 02/17/96 7925-8 ER 1 233 POL AR 02/24/96 7925-10 WR 1 234 GPS-7 03/27/96 7925-8 ER 1 235 MSX 04/24/96 7920-10 WR 1 236 GALAXY 1X 05/24/96 7925A ER 1 237 GPS-26 07/16 /96 7925-9.5 ER 1 9/10/96 141 RTI D .3.2 D elta Failure Narratives The following narratives provide available details about each D elta failure since the beginning of the D elta program. The narratives are numbered to match the flight­ sequence numbers in Section D .3.1. 1. Echo 1,13 M ay 60, Response M ode 4, Flight Phase 2.5: A ttitude control lost during second stage coast period. Third stage spun up, but did not fire. 10. Tiros E, 19 June 62, Response M ode NA , Flight Phase 5: The flight was considered a success, although failure of the BTL guidance system resulted in a propellant­ depletion shutdown of the second stage. The apogee of the final orbit was 175 miles above the planned value and well outside the three-sigma limit of 76 miles. 24. S-66,19 M ar 64, Response M ode 4, Flight Phase 3: Spacecraft did not attain orbit. Third-stage bum of X-248 motor was interrupted after 23 seconds of a planned 42- second bum period. 26. Imp B, 3 Oct 64, Response M ode NA , Flight Phase 5: The flight was considered a partial success, although it failed to reach the desired orbital altitude. The apogee was some 52,590 miles below the planned value of 110,000 miles, but perigee was within 3 miles of the desired value of 105 miles. 28. Tiros I, 22 Jan 65, Response M ode NA , Flight Phase 2 and 5: Loss of W EC O guidance during second-stage burn caused second stage to bum to oxygen depletion. A s a result, spacecraft was inserted into an elliptical rather than a circular orbit. 33. OSO-C , 25 A ug 65, Response M ode 4, Flight Phase 2.5: Third stage ignited after spin up but before separation from second-stage spin table. Payload did not orbit. 34. G EOS A , 6 Nov 65, Response M ode NA , Flight Phase 2 and 5: The flight was considered a success, although failure of the BTL guidance system during second- stage powered flight led to a propellant-depletion shutdown of the stage. A ctual apogee was 436 miles too high, and well outside the three-sigma limit. 38. A E^B, 25 M ay 66, Response M ode NA , Flight Phase 2 and 5: D ue to W EC O guidance failure (ground system locked on side lobe), second stage burned to propellant depletion, some 12 seconds longer than expected. A s a result, the orbital apogee was 800 miles higher than planned. 39. A IM P-D , 1 July 66, Response M ode NA , Flight Phase 2.5 and 5: A lthough an alternate mission was accomplished, primary objectives could not be achieved because excess velocity imparted to the spacecraft prevented insertion of the 9/10/96 142 RTI spacecraft into a lunar orbit. Possible cause was malfunction of the coast-control system after third-stage spinup and separation. 59. Intelsat III A , 18 Sep 68, Response M ode 5, Flight Phase 1: D ue to loss of rate gyro, undamped pitch oscillations began at 20 seconds. Vehicle began a series of violent maneuvers at 59 seconds. D uring the 13-second period while these maneuvers continued, the vehicle pitched down some 270°, then up 210°, and then made a large yaw to the left. A t 72 seconds the vehicle regained control and flew stably in a down and leftward direction until 100 seconds. A t this time, with the main engine against the pitch and yaw stops, the destabilizing aerodynamic forces became so large that quasi-control could no longer be maintained. The first stage broke up at 103 seconds. The second stage was destroyed by the RSO at 110.6 seconds. M ajor pieces impacted about 12 miles downrange and 2 miles left of the flight line. 71. Intelsat III E, 26 July 69, Response M ode NA , Flight Phase 3 and 5: U nknown but anomalous third-stage performance inserted payload into an erroneous orbit. A pogee was some 17,000 miles too low and orbital inclination was 1.5° above planned 28.8° 73. Pioneer E, 27 A ug 69, Response M ode 5, Flight Phase 1: First-stage hydraulics system failed a few seconds before burnout (M EC O). The vehicle pitched down, yawed left, rolled counterclockwise driving all gyros off limits, and then tumbled. Second-stage separation and ignition occurred while the vehicle was out of control. A fter about 20 seconds, the second stage regained control in a yaw-right, pitch-up attitude. The vehicle flew stably in this attitude for about 240 seconds until destroyed by the safety officer at T+484 seconds. 78. Intelsat III G , 22 A pr 70, Response M ode NA , Flight Phase 1 and 5: The flight was considered a success, although low first-stage velocity resulted in a propellant­ depletion shutdown of the second stage. A s a result, the actual apogee was some 2,220 miles below the planned value of 195,400 miles, and well outside three- sigma limits. 85. OSO-H , 29 Sep 71, Response M ode NA , Flight Phase 2 and 5: Stage-2 hydraulic- system failure caused faulty control during second-stage burn. Spacecraft injected initially into an elliptical orbit, but was later maneuvered into a more satisfactory orbit although perigee was still about 93 miles below the planned value. 86. ITOS-B (W TR), 21 Oct 71, Response M ode 4, Flight Phase 2: C ontamination in the oxygen vent valve apparently prevented its proper operation throughout flight. This led to bulkhead rupture during second-stage burn and loss of vehicle control. 9/10/96 143 RTI 96. ITOS-E (W TR), 16 July 73, Response M ode 4T, Flight Phase 2: Pump-motor failure during second-stage burn at 490 seconds resulted in loss of hydraulic pressure, loss of attitude control, and vehicle tumbling. 100. Skynet IIA , 19 Jan 74, Response M ode NA , Flight Phase 4 and 5: Flight was within normal limits until impact point passed through A frica gate. D uring the second burn of the second stage, a short circuit in the second-stage electronics package resulted in an improper spacecraft orbit. The satellite reentered the earth's atmosphere five days later on 24 Jan 74. 101. W ESTA R-B, 13 A pr 74, Response M ode NA , Flight Phase 1: One solid-rocket motor carried to M EC O, but mission was still a complete success. 102. SM S-A , 17 M ay 74, Response M ode NA , Flight Phase 1 and 5: M ission was a partial success, although low first-stage velocity resulted from a liquid oxygen pressure line failure, and a booster shroud that snagged before fully jettisoning. A pogee was some 1,767 miles below the planned value, and well outside three- sigma limits. 130. ESRO-G OES, 20 A pr 77, Response M ode NA , Flight Phase 2.5 and 5: D ue possibly to a short circuit in the second stage or failure in one of the two explosive bolts that hold the stage 2/3 clamp band together, the third stage separated prematurely from the second stage while spinning at only two rpms instead of the normal 97 rpms. A s a result, coning during third-stage burn resulted in a spacecraft apogee nearly 13,000 miles low, and far outside three-sigma limits. 134. O'IS, 13 Sep 77, Response M ode 4, Flight Phase 1: C ore vehicle exploded at 57 seconds due to a burn through on the forward end of the #1 C astor IV motor. 155. D E; 3 A ug 81, Response M ode NA , Flight Phase 2 and 5: Flight was considered a success, although a 260-pound deficiency in fuel loading led to a premature propellant-depletion shutdown of the second bum of the second stage and degradation of final orbit. The inertial velocity at SEC O was 240 ft/sec lower than planned. Final apogee was some 855 miles too low and well outside three-sigma limits. 162. W EST A R-V, 9 June 82, Response M ode NA , Flight Phase 1: Booster performance was low but mission was a success. A pogee and perigee were within three-sigma limits. 178. G OES-G , 3 M ay 86, Response M ode 4, Flight Phase 1: A n electrical short in a control circuit in first-stage relay box caused premature main-engine shutdown at 71 seconds. Vehicle then tumbled and was broken up by aerodynamic forces. RSO sent destruct at approximately 91 seconds. 9/10/96 144 RTI 228. K oreasat, 5 A ug 95, Response M ode NA , Flight Phase 1 and 5: One of three air­ ignited strap-on G EM s did not separate because of a malfunction in the separation explosive transfer system. Failure to drop a G EM motor resulted in depletion of second-stage propellants. A lthough perigee was close to nominal, the apogee was 3,450 nm below the planned value and far outside the 3-sigma limits. 9/10/96 145 RTI D .4 Titan L aunch and Performance H istory The Titan family of launch vehicles was established in 1955, when the A ir Force awarded the M artin C ompany a contact to build a heavy-duty space system. Titan I was the nation's first two-stage IC BM and the first to be silo-based. It proved many structural and propulsion techniques that were later incorporated into Titan II. The Titan II was a heavy-duty missile using storable propellants that became a man-rated space booster for NA SA 's G emini program. Today the Titan II is returning as a space­ launch vehicle with the old IC BM s converted to deliver payloads to orbit. Titan III was the outgrowth of propulsion technology developed in both Titan II and M inuteman ballistic-missile programs. ' Today's Titan vehicles (II, III, and IV) are derived from the earlier Titans. In 1984, the D OD called for a space-launch system that would complement the Space Shuttle to ensure access to space for certain national-security payloads. The Titan IV program began as a short-term program for ten launches from C ape C anaveral A ir Station. H owever, after the C hallenger accident in’ 1986, the program has grown to 41 vehicles. W ith the off-loading of D OD payloads from Shuttle, Titan IV has become D OD 's main access to space for many of its heavy payloads. D esign of the Titan II Space Launch Vehicle (SLV) began at the same time as that for Titan IV. Titan IISLV was developed from refurbished Titanil IC BM s incorporating technology and hardware from the Titan III program. 9/10/96 146 RTI Shortly after the C hallenger accident in 1986, when the U S government decided to offload commercial payloads from the Space Shuttle, M artin M arietta announced plans to develop a Titan III commercial launch vehicle with its own funds. The commercial Titan III is derived from the Titan 34D with a stretched second stage and a bulbous shroud for dual or dedicated payloads. The first commercial Titan III was launched with two communications satellites in D ecember 1989. Table 44 shows a summary of Titan space-vehicle configurations since G emini.1101 _________________ Table 44. Summary of Titan Vehicle C onfigurations_________________ C onfiguration D escription II G emini Titan IIIC BM converted to a man-rated vehicle IIIA Same as Titan II G emini except stretched stages 1 and 2, and an integral Transtage upper stage IIIB Same as IIIA except A gena upper stage instead of Transtage 34B Same as IIIA except stretched stage 1 me Same as IIIA with added 5-segment SRM s IIID Same as IIIC except no upper stage H IE Same as IIID except C entaur upper stage and 14-foot diameter PLF 34D Same as 34B with added S^-segment SRM s. U ses either Transtage or IU S upper stage IISLV Refurbished II IC BM with 10-foot diameter PLF III C ommercialSame as 34D except stretched stage 2, single or dual carrier, enhanced liquid-rocket engines, and 13.1-foot diameter PLF. C an use PA M -D 2, Transtage, or TOS upper stage IV Same as 34D except stretched stages 1 and 2,7-segment SRM or 3- segment SRM U , and 16.7-foot diameter PLF. C an use IU S or C entaur upper stage 9/10/96 147 RTI The entire Titan history through 1995 is depicted rather compactly in bar-graph form in Figure 39. The solid-block portion of each bar indicates the number of launches during the calendar year for which vehicle performance was entirely normal, in so far as could be determined. The clear white parts forming the tops of most bars show the number of launches that were either failures or flights where the launch vehicle experienced some sort of anomalous behavior. Every launch with an entry in the response mode column in Table 45 falls in this category. Such behavior did not necessarily prevent the attainment of some, or even all, mission objectives. Figure 39. Titan Launch Summary 9/10/96 148 RTI D .4.1 Titan L aunch H istory The data in Table 45 summarizes all Titan and Titan-boosted space-vehicle launches since the program began. A launch sequence number is provided in the first column. A launch ID and date are provided in columns 2 and 3. The fourth column indicates the vehicle configuration. The fifth column indicates the launch range. The sixth column indicates the failure-response mode (1 through 5 and NA ) that RTI has determined best describes the failure that occurred. For M ode 3 or 4 failures, a suffix of 'T indicates the vehicle tumbled. Successful launches are indicated by a blank in the Response-M ode column. The seventh column indicates the operational flight phase during which the failure occurred. The last column indicates whether the vehicle configuration is representative of those being launched today. Launches through sequence number 337 were used in the filtering process to estimate failure rate. Table 45. Titan Launch H istory No. Mission/ID L aunch D ate Vehicle Configuration Test Range Response Mode Flight Phase Rep. Conf. 1 Weapons System {WS) 12/20/58 KA-1) ER 0 2 WS 02/03/59 KA-2) ER 0 3 WS 02/06 /59 KA-3) ER 0 4 WS 02/25/59 KA-5) ER 0 5 WS 04/03/59 l(A-4) ER 0 6 WS 05/04/59 l(A-6 ) ER 0 7 । WS 08/14/59 KB-5) ER 1 1 0 8 WS 12/12/59 KC-3) ER 1 1 0 9 WS 02/02/6 0 I (B-7A) ER 0 10 WS 02/05/6 0 ER 4T 1 0 11 WS 02/24/6 0 l(G4) ER 0 12 WS 03/08/6 0 KC-D ER 4 2 0 13 WS 03/22/6 0 KG-5) ER 4 2.5 0 14 WS 04/08/6 0 KC-5) ER 4 2 0 15 WS 04/21/6 0 KG-6 ) ER 0 16 WS 04/28/6 0 KC-6 ) ER 0 17 WS 05/13/6 0 l(G-7) ER 0 18 WS 05/27/6 0 KG-9) . ER 0 19 WS 06 /24/6 0 I (G-10) ER 0 20 WS 07/01/6 0 KJ -2) ER 2 1 0 21 WS . 07/28/6 0 KJ -4) ER 4 1 0 22 WS 08/10/6 0 KJ -7) ER 4 2 0 23 WS 08/30/6 0 KJ -5) ER 0 24 WS 09/28/6 0 KJ -8) ER o 25 WS 09/29/6 0 KG-8) ER 4 1 0 26 WS 10/07/6 0 KW) ER 0 27 WS 10/24/6 0 IK-6 ) ER 0 28 WS 12/20/6 0 KJ -9) ER 4 2 0 29 WS 01/20/6 1 IK-10) ER 4 2 0 30 WS______________________ 02/10/6 1 im................................... ER 0 9/10/96 149 RTI No. Mission/ID L aunch D ate Vehicle Configuration Test Range Response Mode Flight Phase Rep. Conf. 31 WS 02/20/6 1 I (J -13) ER 0 32 WS 03/03/6 1 KJ -12) ER 4 2 0 33 WS 03/28/6 1 KJ -14) ER 0 34 WS 03/31/6 1 I (J -15) ER 4 1 0 35 SILVER SAD D L E 05/03/6 1 WR 0 36 WS 05/23/6 1 I (J -16 ) ER 0 37 WS 06 /24/6 1 I (M-1) ER 4T 2 0 38 WS 07/20/6 1 I (J -18) ER 0 39 WS 07/25/6 1 I (M-2) ER 0 40 WS 08/03/6 1 I (J -19) ER 0 41 WS 09/06 /6 1 I (J -17) ER 0 42 WS 09/07/6 1 l(M-3) ER 5 2 0 43 BIG SAM 09/23/6 1 I (SM-2) WR 0 44 WS 09/28/6 1 l(J -20) ER 0 45 WS 10/06 /6 1 l(M-4) ER 5 2 0 46 WS 10/24/6 1 l(J -21) ER 0 47 WS 11/21/6 1 I (J -22) ER 0 48 WS 11/29/6 1 I (M-5) ER 0 49 WS 12/13/6 1 I (J -23) ER 0 50 WS 12/15/6 1 l(M-6 ) ER 4 2 0 51 D OUBLE MARTINI 01/20/6 2 I (SM-4) WR 4 2 0 52 WS 01/29/6 2 I (M-7) ER 0 53 BLUE GAND ER 02/23/6 2 I (SM-18) WR 4 2 0 54 WS (first Titan II) 03/16 /6 2 II (N-2) ER 0 55 SIL VER TOP 05/04/6 2 I (SM-34) WR 0 56 WS 06 /07/6 2 II (N-1) ER 4 2 0 57 WS 07/11/6 2 II (N-6 ) ER 0 58 WS 07/25/6 2 II (M) ER 4 2 0 59 WS 09/12/6 2 II (N-5) ER 0 6 0 TIGH T BRACELET 10/06 /6 2 I (SM-35) WR 0 6 1 WS 10/12/6 2 II (N-9) ER 0 6 2 WS 10/26 /6 2 II (N-12) ER 0 6 3 YEL LOW J ACKET 12/05/6 2 I (SM-11) WR 4T 2 0 6 4 WS 12/06 /6 2 II (N-11) ER 4 1 0 6 5 WS 12/19/6 2 II (N-13) ER 0 6 6 WS 01/10/6 3 II (N-15) ER 4 2 0 6 7 TEN MEN 01/29/6 3 I (SM-8) WR 0 6 8 WS 02/06 /6 3 II (N-16 ) ER 4 2 0 6 9 AWFUL TIRED 02/16 /6 3 II WR 4T 1 0 70 WS 03/21/6 3 II (N-18) ER 4T 2.5 0 71 YOUNG BL OOD 03/30/6 3 I (SM-3) WR 0 72 H AL F MOON 04/04/6 3 I WR 0 73 RAMP ROOSTER 04/13/6 3 I (SM-1) WR 0 74 WS 04/19/6 3 II (N-21) ER 4 2 0 75 D INNER PARTY 04/27/6 3 II WR 0 76 MARES TAIL 05/01/6 3 I WR 2 1 0 9/10/96 150 RTI No. Mission/ID L aunch D ate Vehicle Configuration Test Range Response Mode Flight Phase Rep. Conf. 77 WS 05/09/6 3 II (N-14) ER 4 2 0 78 FLYING FROG 05/13/6 3 II (N-19) WR 0 79 WS 05/24/6 3 II (N-17) ER 0 80 WS 05/29/6 3 II (N-20) ER 4 1 0 81 TH READ NEED LE 06 /20/6 3 II (N-22) WR 5 2 0 82 SIL VER SPUR 07/16 /6 3 I (SM-24) WR 4 2 0 83 H IGH RIVER 08/15/6 3 I (SM-7) WR 0 84 WS 08/21/6 3 II (N-24) ER 0 85 POL AR ROUTE 08/30/6 3 I (SM-56 ) WR 4 2.5 0 86 D AILY MAIL 09/17/6 3 I (SM-83) WR 0 87 TARTOP 09/23/6 3 II (N-23) WR 0 88 WS 11/01/6 3 II (N-25) ER 0 89 FIRETRUCK 11/09/6 3 II (N-27) WR 4T 1 0 90 FACT RID E 11/14/6 3 I (SM-6 8) WR 0 91 WS 12/12/6 3 II (N-29) ER 0 92 USEFUL TASK 12/16 /6 3 II (N-28) WR 0 93 WS 01/15/6 4 II (N-31) ER 0 94 RED SAILS 01/23/6 4 II (N-26 ) WR 0 95 SAFE COND UCT 02/17/6 4 II WR 0 96 WS 02/26 /6 4 II (N-32) ER 0 97 APPLE PIE 03/13/6 4 II (N-30) WR 0 98 WS 03/23/6 4 II (N-33) ER 0 99 SV: GEMINI GT-1 04/08/6 4 11(0-1) ER 0 100 WS 04/09/6 4 II (N-34) ER 0 101 COBRA SKIN 07/30/6 4 II (B-28) WR 0 102 D OUBL ETALL EY 08/11/6 4 II (B-9) WR 0 103 GENTL E ANNIE 08/13/6 4 II (B-7) WR 0 104 SV (first Titan III) 09/01/6 4 IIIA(6 5-210)/Trans. ER 4 4 0 105 BL ACK WID OW 10/02/6 4 II(B-1) WR 0 106 H IGH RID ER 11/04/6 4 II (B-32) WR 0 107 WEST WIND I 12/08/6 4 I (SM-85) WR 5 1 0 108 SV 12/10/6 4 IIIA (6 5-209)/Trans. ER 0 109 WESTWIND III 01/14/6 5 I (SM-33) WR 4 2 0 110 SV: GEMINI GT-2 01/19/6 5 II (G-2) ER 0 111 SV: L ES-1 02/11/6 5 IIIA (6 5-211)/Trans. ER 0 112 WESTWIND II 03/05/6 5 I (SM-80) WR 4 2 0 113 SV: GEMINI GT-3 03/23/6 5 ll(G-3) ER 0 114 ARTIC SUN 03/24/6 5 II (B-6 0) WR 0 115 BEAR H UG 04/16 /6 5 II (B-45) WR 0 116 CARD D ECK 04/30/6 5 II (B-54) WR 4 1 0 117 SV: L ES-2 05/06 /6 5 IIIA (6 5-214)/Trans. ER 0 118 FRONT SIGH T 05/21/6 5 II (B-51) WR 0 119 SV: GEMINI GT-4 06 /03/6 5 II (G-4) ER 0 120 GOLD FISH 06 /14/6 5 II (B-22) WR 4 2.5 0 121 SV: D UMMY PAYL OAD 06 /18/6 5 IIIC (6 5-215)/Trans. ER 1 122 BUSY BEE 06 /30/6 5 II (B-30)__________________ WR 9/10/96 151 RTI No. Mission/ID L aunch D ate Vehicle Configuration Test Range Response Mode Flight Phase Rep. Conf. 123 L ONG BAL L 07/21/6 5 II (B-6 2) WR 0 124 MAGIC L AMP 08/16 /6 5 II (B-6 ) WR o 125 SV: GEMINI GT-5 08/21/6 5 II (G-5) ER 0 126 NEW ROLE 08/25/6 5 II (B-19) WR 0 127 BOLD GUY 09/21/6 5 II (B-58) WR 4 2 0 128 SV:OV-2,LCS-5 10/15/6 5 IIIC (6 5-212)/Trans. ER NA 4&5 1 129 POWER BOX 10/20/6 5 II (B-33) WR 0 130 RED WAGON 11/27/6 5 II (B-20) WR 0 131 CROSS FIRE 11/30/6 5 II (B4) WR 5 2 0 132 SV: GEMINI GT-7 12/04/6 5 II (G-7) ER 0 133 SV: GEMINI GT-6 A 12/15/6 5 II (G-6 ) ER 0 134 SV: L ES-3,4, OSCAR 4 12/21/6 5 IIIC (6 6 -001)/Trans. ER NA 5 1 135 SEA ROVER 12/22/6 5 II (B-73) WR 4T 2 0 136 WINTER ICE 02/03/6 6 ll(B-87) WR 0 137 BLACK H AWK 02/17/6 6 II (B-6 1) WR 0 138 SV: GEMINI GT-8 03/16 /6 6 II (G-8) ER 0 139 CL OSE TOUCH 03/25/6 6 II (B-16 ) WR 0 140 GOLD RING 04/05/6 6 II (B-50) WR 0 141 L ONG L IGH T 04/20/6 6 II (B-55) WR 0 142 SILVER BULL ET 05/24/6 6 II (B-91) WR 4 2.5 0 143 SV: GEMINI GT-9A 06 /03/6 6 II (G-9) ER 0 144 SV: ID CSP 06 /16 /6 6 IIIC (6 6 -004)/Trans. ER 1 145 SV: GEMINI GT-10 07/18/6 6 II (G-10) ER 0 146 GIANT TRAIN 07/22/6 6 II (B-95) WR 0 147 D AIL Y MAIL 07/29/6 6 IIIB/AGENA D (23B) WR 1 148 SV-ID CSP 08/26 /6 6 IIIC(6 6 -005)/Trans. ER 4T 0 1 149 SV: GEMINI GT-11 09/12/6 6 II (G-11) ER 0 150 BL ACK RIVER 09/16 /6 6 II (B40) WR 0 151 BUSY SCH EME 09/28/6 6 IIIB/AGENA D (23B) WR 1 152 SV-OAR/OV 11/03/6 6 IIIC (6 6 -002)/Trans. ER 153 SV:GEMINIGT-12 11/11/6 6 II (G-12) ER 0 154 BUBBLE GIRL 11/24/6 6 II (B-6 8) WR 0 155 BUSy SKYR0CKET 12/14/6 6 IIIB/AGENA D (23B) WR 1 156 SV-ID CSP/L ES/D ATS 01/18/6 7 IIIC (6 6 -006 )/Trans. ER 1 157 BUSY PAL EFACE 02/24/6 7 IIIB/AGENA D (23B) WR 1 158 GIFT H ORSE 03/17/6 7 II (8-76 ) WR 0 159 GL AMOUR GIRL 04/12/6 7 II (B-81) WR 4T 2 0 16 0 BUSY TAILOR 04/26 /6 7 IIIB/AGENA D (23B) WR 4 2 1 16 1 SV-VEL A/RSCH 04/28/6 7 IIIC (6 6 -003)Trans. ER 1 16 2 BUSY PLAYMATE 06 /20/6 7 IIIB/AGENA D (23B) WR 1 16 3 BUGGY WH EEL 06 /23/6 7 II (B-70) WR 0 16 4 SV-ID CSP 07/01/6 7 IIIC(6 6 -007)/Trans. ER 1 16 5 AFSC 08/16 /6 7 IIIB/AGENA D (23B) WR 1 16 6 GL OWING BRIGH T 09/11/6 7 II (B-21) WR 0 16 7 AFSC 09/19/6 7 IIIB/AGENA D (23B) WR 1 16 8 AFSC ___________ 10/25/6 7 IIIB/AGENA D (23B) WR 1 9/10/96 152 RTI No. Mission/ID L aunch D ate Vehicle Configuration Test Range Response Mode Flight Phase Rep. Conf. 16 9 AFSC 12/05/6 7 IIIB/AGENA D (23B) WR 1 170 AFSC 01/18/6 8 IIIB/AGENA D (23B) WR 1 171 GL ORY TRIP 4T 02/28/6 8 II (M8) WR 0 172 AFSC 03/13/6 8 IIIB/AGENA D (23B) WR 1 173 GL ORY TRIP 10T 04/02/6 8 II (B-36 ) WR 0 174 AFSC 04/17/6 8 IIIB/AGENA D (23B) WR 1 175 AFSC 06 /05/6 8 IIIB/AGENA D (23B) WR 1 176 GL ORY TRIP 8T 06 /12/6 8 II (B-82) WR 0 177 SV-ID CSP 06 /13/6 8 IIIC (6 6 -009)Trans. ER 1 178 AFSC 08/06 /6 8 IIIB/AGENA D (23B) WR 1 179 GL ORY TRIP 18T 08/21/6 8 II (B-53) WR 0 180 AFSC 09/10/6 8 IIIB/AGENA D (23B) WR 1 181 SV-L ES/OV 09/26 /6 8 IIIC (6 5-213)Trans. ER 1 182 AFSC 11/06 /6 8 IIIB/AGENA D (23B) WR 1 183 GL ORY TRIP 26 T 11/19/6 8 II (B-3) WR 0 184 AFSC 12/04/6 8 IIIB/AGENA D (23B) WR 1 185 AFSC 01/22/6 9 IIIB/AGENA D (23B) WR 1 186 SV-TACCOM 02/09/6 9 IIIC-17/Trans. ER 1 187 AFSC 03/04/6 9 IIIB/AGENA D (23B) WR 1- 188 AFSC . 04/15/6 9 IIIB/AGENA D (23B) WR 189 GL ORY TRIP 39T 05/20/6 9 II WR 0 190 SV-VEL A/OV 05/23/6 9 IIIC-15/Trans. ER 1 191 AFSC 06 /03/6 9 IIIB/AGENA D (23B) WR 1 192 AFSC 08/23/6 9 IIIB/AGENA D (23B-1) WR 1 193 AFSC 10/24/6 9 IIIB/AGENA D (23B-2) WR 1 194 AFSC 01/14/70 IIIB/AGENA D (23B-3) WR 1 195 SV-VEL A 04/08/70 IIIC-18/Trans. ER 1 196 AFSC 04/15/70 IIIB/AGENA D (23B-4) WR 1 197 AFSC 06 /25/70 IIIB/AGENA D (23B-5) WR 1 198 ^ 08/18/70 IIIB/AGENA D (23B-6 ) WR 1 199 AFSC 10/23/70 IIIB/AGENA D (23B-7) WR 1 200 SV-D OD 11/06 /70 IIIC-19/Trans. ER NA 3.5 & 5 . 1 201 AFSC 01/21/71 IIIB/AGENA D (23B-8) WR 1 202 AFSC 03/20/71 IIIB/AGENA D (33B-1) WR 1 203 AFSC 04/22/71 IIIB/AGENA D (23B-9) WR 1 204 SV-D OD 05/05/71 IIIC-20/Trans. ER 1 205 AFSC 06 /15/71 IIID (23D -1) WR 1 206 M1-17 06 /20/71 II (B-12) WR 0 207 AFSC 08/12/71 IIIB/AGENA D (24B-1) WR 1 208 M2-1 08/27/71 II (B-100) WR 0 209 AFSC 10/23/71 IIIB/AGENA D (24B-2) WR 1 210 SV-D OD 11/02/71 IIIC-21/Trans. ER 1 211 AFSC 01/20/72 H ID (23D -2) WR 1 212 AFSC 02/16 /72 IIIB/AGENA D (33B-2) WR 4 3 1 213 SV-D OD 03/01/72 IIIC-22/Trans. ER 1 214 AFSC____________________ 03/17/72 IIIB/AGENA D (24B-3) WR 1 9/10/96 153 RTI No. Misslon/ID L aunch D ate Vehicle Configuration Test Range Response Mode Flight Phase Rep. || Conf. 215 AFSC 05/20/72 IIIB/AGENAD (24B-4) WR 1 216 M2-10 05/24/72 II (B-46 ) WR 0 217 AFSC 07/07/72 H ID (23D -5) WR 1 218 AFSC 09/01/72 IIIB/AGENAD (24B-5) WR 1 21-9 AFSC 10/10/72 H ID (23D -3) WR 1 220 M2-14 10/11/72 II (B-78) WR 0 221 AFSC 12/21/72 IIIB/AGENA D (24B^6 ) WR 1 222 AFSC 03/09/73 H ID (23D -6 ) WR 1 223 AFSC 05/16 /73 IIIB/AGENA D (24B-7) WR 1 224 SV-D SP 06 /12/73 IIIC-24/Trans. ER 1^ AFSC 06 /26 /73 IIIB/AGENA D (24B-9) WR 1 226 AFSC 07/13/73 H ID (23D -7) WR 1 227 AFSC 08/21/73 IIIB/AGENA D (33B-3) WR 1 228 AFSC 09/27/73 IIIB/AGENA D (24B-8) WR 1 229 M2-27 10/05/73 II WR 0 230 AFSC 11/10/73 H ID (23D -8) WR 1 231 SV-D SCS 12/13/73 H IC-26 /Trans. ER 1 232 SV-VIKING 02/11/74 IIIE/CENT. D -1T (TC-1) ER 4 3 1 233 AFSC 02/13/74 IIIB/AGENA D (24B-10) WR 1 234 M2-31 03/01/74 II WR 0 235 AFSC 04/10/74 H ID (23D -9) WR 1 236 SV-ATS-F 05/30/74 H IC-9/Trans. ER 1 237 AFSC 06 /06 /74 IIIB/AGENA D (24B-11) WR 1 238 AFSC 08/14/74 IIIB/AGENA D (24B-12) WR 1 239 AFSC 10/29/74 H ID (23D 4) WR 1 240 SV-H EL IOS-A(TC-2) 12/10/74 H IE/CENT-1T (23E-2) ER 1 241 SOFT-1 01/09/75 II WR 0 242 AFSC 03/09/75 IIIB/AGENA D (34B-1) WR 1 243 AFSC 04/18/75 IIIB/AGENA D (24B-14) WR 1 244 SV-D SCS 05/20/75 IIIC-7/Trans. ER NA 2.5 1 245 AFSC 06 /08/75 H ID (23D -10) WR 1 246 D G-2 08/07/75 II WR 0 247 SV-Viking/Mars (TC4) 08/20/75 IIIE/CENT. D -1T (23E-4) ER 1 248 SV-Viking/Mars (TC-3) 09/09/75 IIIE/CENT. D -1T(23E-3) ER 1 249 AFSC 10/09/75 IIIB/AGENA D (24B-10) WR 1 250 AFSC 12/04/75 H ID (23D -13) WR 1 251 D G-4 12/04/75 II WR 0 252 SV-D SP 12/14/75 IIIC-29/Trans. ER NA 5 1 253 SV-H ELIOS-B (TC-5) 01/15/76 IIIE/CENT. D -1T(23E-5) ER 1 254 SV-LES/SOL RAD 03/14/76 IIIC-30/Trans. ER 1 255 AFSC 03/22/76 IIIB/AGENA D (23B-18) WR 1 256 AFSC 06 /02/76 IIIB/AGENA D (34B-5) WR 1 257 SV-D SP 06 /25/76 IIIC-28/Trans. ER 1 258 ITF-1 06 /27/76 II WR 0 259 AFSC 07/08/76 H ID (23D -14) WR 1 26 0 AFSC 08/06 /76 IIIB/AGENA D (34B-6 ) WR 1 9/10/96 154 RTI No. Mission/ID L aunch D ate Vehicle Configuration Test Range Response Mode Flight Phase IS." Conf. 26 1 AFSC 09/15/76 IIIB/AGENA D (24B-17) WR NA 2 1 26 2 AFSC 12/19/76 H ID (23D -15) WR 1 26 3 SV-D SP 02/06 /77 IIIC-23/Trans. ER 1 26 4 AFSC 03/13/77 IIIB/AGENA D (24B-19) WR 1 26 5 SV-D SCS 05/12/77 IIIC-32/Trans. ER 1 26 6 AFSC 06 /27/77 H ID (23D -17) WR 1 26 7 SV-VOYAGER (TC-7) 08/20/77 IIIE/CENT.D -1T(23E-7) ER 1 26 8 SV-VOYAGER (TC-6 ) 09/05/77 |H i/CENT.D -1T(23E-6 ) ER NA 2 1 26 9 AFSC 09/23/77 IIIB/AGENA D (24B-23) WR 1 270 AFSC 02/24/78 IIIB/AGENA D (34B-2) WR 1 271 AFSC 03/16 /78 H ID (23D -20) WR 1 272 SV-D SCS 03/25/78 IIIC-35/Trans. ER 4T 2 1 273 SV-D OD 06 /10/78 IIIC-33/Trans. ER 1 274 AFSC 06 /14/78 H ID (23D -18) WR 1 275 AFSC 08/04/78 IIIB/AGENA D (34B-7) WR 1 276 SV-D SCS 12/13/78 IIIC-36 /Trans. ER 1 277 AFSC 03/16 /79 H ID (23D -21) WR 1 278 AFSC 05/28/79 IIIB/AGENA D (24B-25) WR 1 279 SV-D SP 06 /10/79 H IC-23C-13/rrans. ER 1 280 SV-D OD . 10/01/79 H IC-23C-16 /Trans. ER 1 281 SV-D SCS 11/21/79 IH C-23C-19/Trans. ER 1 282 AFSC 02/06 /80 H ID (23D -19) WR 1 283 AFSC 06 /18/80 H ID (23D -16 ) WR 1 284 AFSC - 12/13/80 IIIB/AGENA D (34B-3) WR 1 285 AFSC 02/28/81 IIIB/AGENA D (24B-24) WR 1 286 SV-D OD 03/16 /81 IIIC-23C-22/Trans. ER 1 287 AFSC 04/24/81 IIIB/AGENA D (34B-8) WR 1 288 AFSC 09/03/81 H ID (23D -22) WR 1 289 SV-D OD 10/31/81 IH C-23C-21/rrans. ER 1 290 AFSC 01/21/82 IIIB/AGENA D (24B-26 ) WR 1 291 SV-D OD 03/06 /82 li!C-23C-20/Trans. ER 1 292 AFSC 05/11/82 H ID (23D -24) WR 1 293 SV-D SCS 10/30/82 34D -01/IUS ER 1 .294 AFSC 11/17/82 H ID (23D -23) WR 1 295 AFSC 04/15/83 IIIB/AGENA D (24B-27) WR 1 296 AFSC 06 /20/83 34D -5 WR 1 297 AFSC 07/31/83 IIIB/AGENA D (34B-9) WR 298 SV-D OD 01/31/84 34D -10/Trans. ER 1 299 SV-D OD 04/14/84 34D -11/Trans. ER 1 300 AFSC 04/17/84 IIIB/AGENA D (24B-28) WR 1 301 AFSC 06 /25/84 34D -4 WR 1 302 AFSC 08/28/84 IIIB/AGENA D (34B-4) WR 1 303 AFSC 12/04/84 34D -6 WR 1 304 SV-D OD 12/22/84 34D -13/Trans. ER 1 305 AFSC 02/07/85 IIIB/AGENA D (34B-10) WR 1 306 AFSC 08/28/85 34D -7- WR 4T 1 1 9/10/96 155 RTI No. Mission/ID L aunch D ate Vehicle Configuration Test Range Response Mode Flight Phase Rep. Conf. 307 AFSC 04/18/86 34D -9 WR 4 0 1 308 AFSC 02/11/87 IIIB/AGENAD (34B-11) WR 1 309 AFSC 10/26 /87 34D -15 WR 1 310 SV-D OD 11/29/87 34D -8/Trans. ER 1 311 SV-D OD 09/02/88 34D -3/Trans. ER NA 5 1 312 AFSC 09/05/88 II/SL V (23G-1) WR 1 313 AFSC 11/06 /88 34D -14 WR 1 314 SV-D OD 05/10/89 34D -16 /Trans. ER 1 315 SV (first T-IV) 06 /14/89 IV-1/IUS ER NA 1 1 316 SV-D OD 09/04/89 34D -2/Trans. ER 1 317 AFSC 09/05/89 II/SL V (23G-2) WR 1 318 SV-J APAN/UK 01/01/90 III ER 1 319 SV-INTELSATVI 03/14/90 III ER NA 2.5 & 5 1 320 SV-D OD 06 /08/90 IV4 ER 1 321 SV-INTELSATVI 06 /23/90 III ER 1 322 SV-D OD 11/13/90 IV-6 /IUS ER 1 323 AFSC 03/08/91 IV WR 1 324 AFSC 11/17/91 IV WR 1 325 AFSC 04/25/92 II/SL V WR 1 326 SV-MARSOBS. 09/25/92 III ER 1 327 AFMC 11/28/92 IV WR 1 328 AFMC 08/02/93 IV(K-11) WR 4 0 1 329 L AND SAT6 10/05/93 II/SL V WR 4 2 1 330 CLEMENTINE 01/25/94 II/SLV WR 1 331 SV-MILSTAR 02/07/94 TIV-CENTAUR (K-10) ER 1 332 SV-D OD 05/03/94 TIV-CENTAUR (K-7) ER 1 333 SV-D OD 08/27/94 TIV-CENTAUR (K-9) ER 1 334 SV-D OD 12/22/94 IV-IUS (K-14) ER 1 335 SV-D OD 05/14/95 TIV-CENTAUR (K-23) ER 1 336 SV-D OD 07/10/95 TIV-CENTAUR (K-19) ER 1 337 SV-MILSTAR 11/06 /95 TIV-CENTAUR (K-21) ER 1 338 D OD 04/24/96 TIV-CENTAUR (K-16 ) ER 1 D OD ____________________ 07/02/96 TIV-NUS(K2) ER sass^ .... 1 9/10/96 156 RTI D .4.2 Titan Failure Narratives The following narratives provide available details about each Titan failure since the beginning of the Titan I program in 1959. The narratives are numbered to match the flight-sequence numbers in Section D .4.1. 7. B-5, 14 A ug 59, Response M ode 1, Flight Phase 1: U mbilicals were prematurely pulled from missile resulting in engine shutdown and impact on pad. 8. C -3, 12 D ec 59, Response M ode 1, Flight Phase 1: M issile destroyed itself just before liftoff. 10. C -4, 5 Feb 60, Response M ode 4T, Flight Phase 1: W hile pitch program was in progress, a structural failure occurred in transition section. Nose cone broke off, and missile lost aerodynamic stability. Shortly after, an explosion and fire destroyed the missile. 12. C -l, 8 M ar 60, Response M ode 4, Flight Phase 2: Failure of gas-generator valve to open prevented Stage-II ignition. 13. G -5, 22 M ar 60, Response M ode 4, Flight Phase 2.5: Premature shut down of vernier engines resulted in impact 38 miles short of target. 14. C -5, 8 A pr 60, Response M ode 4, Flight Phase 2: A lthough Stage-I performance was low, Stage II successfully separated and ignited. A ll data were lost about 50 seconds later, apparently due to malfunction of Stage II turbopump. 20. J-2, 1 Jul 60, Response M ode 2, Flight Phase 1: Shortly after launch, hydraulic power to engine actuators was lost so control could not be maintained. The missile veered northwest and pitched down (Flight azimuth was 105.97°). M issile was destroyed by RSO 11 seconds after liftoff. 21. J-4, 28 July 60, Response M ode 4, Flight Phase 1: Stage I thrusting flight was terminated prematurely at 101 seconds (Nominal, 136 seconds). Stage II engine did not start, apparently because the auxiliary turbopumps did not receive sufficient head pressure to effect a successful start. 22. J-7, 10 A ug 60, Response M ode 4, Flight Phase 2: Stage II engine shutdown 0.17 seconds early and solo vernier operation did not occur. Impact was 107 miles short of target. 25. G -8, 29 Sep 60, Response M ode 4, Flight Phase 1: Stage I shut down prematurely when a low-level sensor malfunctioned and ceased to be locked out. Stage II performed properly but shutdown prematurely due to propellant depletion. The impact was some 3600 miles short of the 8700-mile target point. 9/10/96 157 RTI 28. J-9,20 D ec 60, Response M ode 4, Flight Phase 2: No Stage-II ignition due to failure of gas generator to start. 29. J-10, 20 Jan 61, Response M ode 4, Flight Phase 2: No' Stage-II operation due to erroneous signal that appeared at umbilical disconnect. Impact some 420 miles downrange. 32. J-12,3 M ar 61, Response M ode 4, Flight Phase 2: Stage-II terminated prematurely after 54-second burn, apparently due to failure of pump drive assembly. Impact was 730 miles downrange. 34. J-15,31 M ar 61, Response M ode 4, Flight Phase 1: Booster shut down prematurely at 74 seconds. M issile subsequently tumbled and broke up. 37. M -l, 24 Jun 61, Response M ode 4T, Flight Phase 2: Stage II engine shut down prematurely after 12 seconds of operation due to loss of Stage II hydraulic power. Loss of hydraulic power occurred during Stage I flight, so failure led to loss of control of sustainer and vernier actuators, producing excessive missile motion and tumbling. 42. M -3,7 Sep 61, Response M ode 5, Flight Phase 2: A transient in guidance computer at 218.35 seconds (SEC O at 297.7 seconds) caused impact 20 miles short and 2.8 miles left of target. 45. M -4,6 Oct 61, Response M ode 5, Flight Phase 2: A one-bit error in the W velocity accumulation caused impact 86 miles short and 14 miles right of target. 50. M -6,15 D ec 61, Response M ode 4, Flight Phase 2: Start signal for Stage II was not generated. Stage II did not ignite. 51. I, 20 Jan 62, Response M ode 4, Flight Phase 2: M issile self-destructed, apparently after Stage 2 failed to ignite. A backup automatic fuel-cutoff signal was sent at 248 Seconds. 53. 1,23 Feb 62, Response M ode 4, Flight Phase 2: M issile self-destructed, apparently after Stage 2 failed to ignite. A backup automatic fuel cutoff signal was sent at 240 Seconds. 56. N-l, 7 Jun 62, Response M ode 4, Flight Phase 2: Sustainer engine performance was subnormal due to reduced oxidizer flow through the gas generator. RSO terminated flight after a prolonged sustainer burn. Impact only 1100 miles downrange. 58. N-4,25 July 62, Response M ode 4, Flight Phase 2: A fter about 60 seconds of Stage II burn, a fuel leak between the thrust chamber valve and the injector resulted in a 9/10/96 158 RTI 50% reduction of sustainer thrust for remainder of Stage II operation. Impact was 2888 miles short of target. 63. I (Yellow Jacket), 5 D ec 62, Response M ode 4T, Flight Phase 2: M issile was command destructed at 250 seconds. No other data available. 64. N-ll, 6 D ec 62, Response M ode 4, Flight Phase 1: Stage I shut down 11.4 seconds early. A s a result, no inertial velocity-dependent discretes were issued and Stage II shut down prematurely, apparently due to an oxidizer bootstrap-line failure. 66. N-15, 10 Jan 63, Response M ode 4, Flight Phase 2: Stage II flight was terminated by backup SEC O approximately 34 seconds after ignition because low thrust caused velocity to fall below performance criteria. C ause of low thrust was reduced oxidizer flow through the gas-generator injector. Impact only 556 miles downrange. 68. N-16, 6 Feb 63, Response M ode 4, Flight Phase 2: Oxidizer depletion prior to normal SEC O resulted in impact 71 miles short of target. 69. N-7 (A wful Tired), 16 Feb 63, Response M ode 4T, Flight Phase 1: M issile self­ destructed at 56 seconds at an altitude of 18,000 feet due to loss of roll control. Failure was caused by improper umbilical release at launch and subsequent loss of vehicle electrical control. 70. N-18, 21 M ar 63, Response M ode 4T, Flight Phase 2.5: A lthough vernier ignition was normal, vernier #2 received no commands, and gimbaled erratically 2.8 seconds later. R/V attitude was incorrect at separation so that impact was 4 to 5 miles short of target. 74. N-21, 19 A pr 63, Response M ode 4, Flight Phase 2: Stage II engine shut down prematurely due to oxidizer bootstrap-line failure. 76. Titan I (M ares Tail), 1 M ay 63, Response M ode 2, Flight Phase 1: The missile was erratic from liftoff as one engine either failed at liftoff or shutdown immediately thereafter. The missile rose about 50 feet, then fell uprange from the launch pad about 7.5 seconds after liftoff. 77. N-14,9 M ay 63, Response M ode 4, Flight Phase 2: Oxidizer depletion due to a leak resulted in premature Stage II shutdown and impact short of target. 80. N-20, 29 M ay 63, Response M ode 4, Flight Phase 1: A fuel leak in Stage I engine compartment at ignition caused a fire that spread through the engine compartment. Stage I destroyed itself at 52 seconds. Stage II was destroyed by RSO. 9/10/96 159 RTI 81. Titan II (Thread Needle), 20 June 63, Response M ode 5, Flight Phase 2: Flight appeared normal until BEC O at about 146 seconds. The staging event seemed abnormally long, due to' low second-stage thrust that remained considerably below normal thereafter because of reduced oxidizer flow through the gas­ generator injector. The vehicle nevertheless followed closely to the intended ground track, albeit well behind schedule. A t about 480 seconds (and some three minutes behind schedule), the missile began a slow turn to the left. A SEC O indication was noted about 10 seconds later. D estruct was sent at 532 seconds after all track was lost. 82. Titan I (Silver Spur), 16 July 63, Response M ode 4, Flight Phase 2: The flight was normal through first-stage cutoff. Separation occurred but the second-stage failed to ignite. 85. Titan I (Polar Route), 30 A ug 63, Response M ode 4, Flight Phase 2.5: The flight appeared normal through the first and second-stage thrusting periods. A t SEC O the vernier engines also shut down, apparently due to shutdown of the gas generator. 89. II (Fire Truck), 9 Nov 63, Response M ode 4T, Flight Phase 1: M issile tumbled out of control at 130 seconds, then broke up. 104. IIIA (65-210), 1 Sep 64, Response M ode 4, Flight Phase 4: Nominal mission through first transtage burn. Transtage propellant-tank pressurization system failed with resultant reduction in thrust. Vehicle impacted about 2700 miles downrange. 107. Titan I (W est W ind I), 8 D ec 64, Response M ode 5, Flight Phase 1: A first-stage power-level malfunction combined with guidance deviations caused the missile to drift far to the left, then over-correct far to the right, passing north of M idway Is. No other data available. 109. Titan I (W est W ind III), 14 Jan 65, Response M ode 4, Flight Phase 2: First-stage flight was apparently normal, but second stage failed to ignite. 112. Titan I (W est W ind II), 5 M ar 65, Response M ode 4, Flight Phase 2: M issile impacted on azimuth about 80 miles short of target due to propellant depletion. 116. Titan I (C ard D eck), 30 A pr 65, Response M ode 4, Flight Phase 1: Flight appeared normal until around 100 seconds when the IP slowed and then stopped due to a turbopump failure. The missile self-destructed at about 115 seconds with the impact point about 115 miles offshore. 120. Titan II (G old Fish), 14 Jun 65, Response M ode 4, Flight Phase 2.5: Vehicle apparently failed during-the vernier solo phase due to loss of a vernier nozzle. 9/10/96 160 RTI 127. Titan II (Bold G uy), 21 Sep 65, Response M ode 4, Flight Phase 2: A fter a normal first-stage flight, the second stage was shut down immediately after start by an erroneous guidance command. 128. IIIC (65-212), 15 Oct 65, Response M ode NA , Flight Phase 4 and 5: Normal mission through transtage second ignition and burn. One chamber of transtage engine failed to shutdown completely, resulting in a pitch-up deviation, loss of control, vehicle tumbling, and an unplanned orbit. 131. Titan II (C ross Fire), 30 Nov 65, Response M ode 5, Flight Phase 2: Trouble apparently began between 208 and 214 seconds when the rate and track beacons were lost. The radar tracked till about 360 - 380 seconds, indicating a ballistic- type trajectory veering to the right. Loss of control was due to a fuel leak at the crossover manifold. 134. IIIC (66-001), 21 D ec 65, Vehicle 8, Response M ode NA , Flight Phase 5: Nominal mission through transtage second bum shutdown. A ttitude control system engine failed to shutdown following vernier bum with resulting fuel depletion and loss of attitude control. 135. Titan II (Sea Rover), 22 D ec 65, Response M ode 4T, Flight Phase 2: Flight was apparently normal until some point well into second-stage bum. Track then indicated erratic movement left of nominal, then right of nominal, but with little downrange movement of the IP. A utomatic fuel cutoff was sent at 396 seconds. Failure resulted from improper rigging of sustainer actuator that exceeded control-system capability. 142. Titan II (Silver Bullet), 24 M ay 66, Response M ode 4, Flight Phase 2.5: Flight was normal except that R/V did not separate, causing a 20-mile uprange miss. 148. IIIC (66-005), 26 A ug 66, Vehicle 12, Response M ode 4T, Flight Phase 0: Payload fairing failed during Stage-0 powered flight The failure at 79 seconds resulted in violent maneuvering and self destruct (ISD S). 159. Titan II (G lamour G irl), 12 A pr 67, Response M ode 4T, Flight Phase 2: First-stage flight was normal. A bout 15 seconds after second-stage ignition, failure of the yaw-rate gyro resulted in violent roll and pitch maneuvers. M issile impacted about 660 miles downrange. 160. IIIB/A gena D (Busy Tailor), 26 A pr 67, Response M ode 4, Flight Phase 2: Flight appeared normal through first-stage cutoff and separation. A bout 15 seconds into the second stage, a fuel-line blockage resulted in a drop in chamber pressure that reduced the thrust to about half its normal level. A s a result, the velocity eventually stopped increasing. The IP moved slightly farther downrange and remained on azimuth until loss of signal at 300 seconds. Impact was about 600 miles downrange. 9/10/96 161 RTI 200. IIIC -19, 6 Nov 70, Vehicle 19, Response M ode NA , Flight Phase 3.5 and 5: A ll booster systems performed essentially as planned. Transtage experienced a guidance anomaly during coast prior to second burn resulting in an improper orbit. 212. IIIB/A gena D (A FSC ), 16 Feb 72, Response M ode 4, Flight Phase 3: A fter an apparently normal Titan III B boost phase, the A gena failed to ignite. The payload impacted about 1500 miles downrange. 232. Titan H IE, #E1, 11 Feb 74, Response M ode 4, Flight Phase 3: A ll Titan booster functions and C entaur separation were properly performed. C entaur stage failed to ignite. 244. TIIIC -25,20 M ay 75, Vehicle 25, Response M ode NA , Flight Phase 2.5: A ll systems performed satisfactorily through Stage II/III separation. A bout 230 milliseconds after staging discrete was issued, the IM U power supply failed. Transtage then tumbled and the first transtage burn failed to occur leaving transtage and attached payload in the parking orbit. 252. TIIIC -29, 14 D ec 75, Vehicle 29, Response M ode NA , Flight Phase 5: A ll launch vehicle objectives were met. H owever, satellite propulsion system malfunctioned putting satellite in uncontrollable position with no possibility of restoring mission capability. 261. IIIB/A gena D (A FSC ), 15 Sep 76, Response M ode 4, Flight Phase 2: The stage-2 engine failed to respond to shutdown commands and thus burned to propellant depletion. C ause was thought to be a hard contaminant that blocked the fuel valve. 268. 23E-6/C entaur D -1T, 5 Sep 77, Response M ode NA , Flight Phase 2: Flight was regarded as a success, although the second-stage velocity was low, probably due to a detached line diffuser lodged on top of the prevalve. 272. TIIIC -17, 25 M ar 78, Vehicle 35, Response M ode 4T, Flight Phase 2: Vehicle performance was satisfactory until 16.4 seconds beyond Stage-2 start. A t this time the Stage-2 hydraulic system began and continued over-pressurizing until the system burst after 125 seconds of Stage-2 operation. The pressure then dropped to zero, the vehicle tumbled out of control, and guidance shut down the second stage after detecting negative acceleration. The RSO sent arm at 629 seconds and destruct at 630 seconds. 306. 34D (A FSC ), 28 A ug 85, Response M ode 4T, Flight Phase 1: The first-stage engine suffered three separate major anomalies: (1) during subassembly-2 (S/ A -2) start transient (110 sec), a large oxidizer leak of 165 Ib/sec occurred in the oxidizer suction line; (2) at 213 seconds, an internal fuel leak of 30 lb/sec occurred in S/A -l downstream of the combustion chamber and created a vehicle side force; (3) the 9/10/96 162 RTI S/A -l shut down at 213 sec due to failure of its turbopump assembly. The vehicle continued flight till 221 seconds when erratic attitude rates were noted. A t 229 seconds, the impact point stopped. A t 257 seconds, the pressure dropped to zero in the stage-1 thrust-chamber assembly 2. A t the same time, stages 1 and 2 separated as stage 2 ignited. A fter this time, stage-2 attitude rates were erratic. D estruct was sent by the RSO at 273 seconds. 307. 34D (A FSC ), 18 A pr 86, Response M ode 4, Flight Phase 0: A t about 8.8 seconds after liftoff, the insulation and case of SRM No. 2 debonded resulting in case rupture immediately thereafter. The core vehicle was destroyed by fragments from the ruptured motor. A uto-destruct was activated on SRM -1 at 9.0 seconds. 311. 34D -3/Transtage, 2 Sep 88, Response M ode NA , Flight Phase 5: Transtage pressurization system failed due to damage to the upper portion of the transtage fuel tank and pressurization lines. A leak of 1,340 pounds occurred during park orbit, and a large helium-tank gas leak occurred during transtage first burn. Not enough helium was left in system to allow start of second burn. The payload was left in a geostationary transfer orbit. 315. Titan IV-l/IU S, 14 June 89, Response M ode NA , Flight Phase 1: Late in Stage-1 burn, one of the engines failed and shut down. The other engine was able to gimbal sufficiently to maintain control until propellant depletion. Trajectory inaccuracies were compensated for during Stage-2 bum, and the mission was a success. 319. C ommercial Titan, 14 M ar 90, Response M ode NA , Flight Phase 2.5 and 5: Boost phase was satisfactory. The payload separation system was designed for two satellites and had two discrete outputs from the missile guidance computer (M G C ), but for this mission it carried only a single satellite. The wiring team miswired the harness, which connected the M G C payload-separation discretes to the payload separation device, so the satellite never received the separation signal. PK M and satellite did not separate from Stage II resulting in low-earth elliptical orbit. G round controllers were able to separate satellite hours later but PK M remained attached to Stage II. 328. IV, 2 A ug 93, Response M ode 4, Flight Phase 0: A leak occurred in SRM #1 at 99.9 seconds that rapidly enveloped the vehicle in propellant gases. A pproximately 1.6 seconds later the vehicle blew up and disintegrated, apparently due to activation of the inadvertent-separation destruct system. D estruct was transmitted at 104.5 seconds. 329. II/SLV (Landsat 6), 5 Oct 93, Response M ode 4, Flight Phase 2: Following a successful Titan-II second-stage bum and after payload separation, the apogee­ kick motor failed to ignite and circularize the highly-elliptical orbit. The Landsat payload and Titan II followed a ballistic trajectory back into the atmosphere where burnup occurred. 9/10/96 163 RTI D .5 Thor L aunch and Performance H istory (Not Including D elta) The entire Thor history is depicted rather compactly in bar-graph form in Figure 40. The solid-black portion of each bar indicates the number of launches during the calendar year for which vehicle performance was entirely normal, in so far as could be determined. The clear white parts forming the tops of most bars show the number of launches that were either failures or flights where the launch vehicle experienced some sort of anomalous behavior. Every launch with an entry in the response mode column of Table 46 falls in this category. Such behavior did not necessarily prevent the attainment of some, or even all, mission objectives. L aunch Year Figure 40. Thor Launch Summary D .5.1 Thor and Thor-Boosted L aunch H istory The data in Table 46 summarize all Thor and Thor-boosted space-vehicle launches since the program began. A launch sequence number is provided in the first column. A launch ID and date are provided in columns 2 and 3. The fourth column indicates the vehicle configuration. The fifth column indicates the launch range. The sixth column indicates the failure-response mode (1 through 5 and NA ) that RTI has determined best describes the failures that occurred. For M ode 3 or 4 failures, a suffix of T indicates the vehicle tumbled. Successful launches are indicated by a blank in the Response- 9/10/96 164 RTI M ode column. The seventh column indicates the operational flight phase during which the failure occurred. The last column indicates whether the vehicle configuration is representative of those being launched today. Table 46. Thor Launch H istory No. Mission/ID L aunch D ate Vehicle Configuration Test Range Response Mode Flight Phase Rep. Conf. 1 Weapons System (WS) 01/25/57 101 ER 1 1 0 2 WS 04/19/57 102 ER 4 1 0 3 WS 05/21/57 103 ER 1 1 0 4 WS 08/30/57 104 ER 4T 1 0 5 WS 09/20/57 105 ER 4 1 0 6 WS 10/03/57 107 ER 1 1 0 7 WS 10/11/57 108 ER 4 1 0 8 WS 10/24/57 109 ER 0 9 WS 12/07/57 112 ER 5 1 0 10 WS 12/19/57 113 ER 4 1.5 0 11 WS 01/28/58 114 ER 5 1 0 12 WS 02/28/58 120 ER 4 1 0 13 WS 04/19/58 121 ER 1 1 0 14 WS 04/23/58 ABL E I (116 ) ER 4 1 0 15 WS 06 /04/58 115 ER 0 16 WS 06 /13/58 122 ER 0 17 WS 07/11/58 ABL E I (118) ER 0 18 WS 07/12/58 123 ER 4 1 0 19 WS 07/23/58 ABL E I (119) ER 0 20 WS 07/26 /58 126 ER 4 1 0 21 WS 08/06 /58 117 ER 0 22 PIONEER 08/17/58 ABL E I (127) ER 4 1 0 23 PIONEER-I 10/11/58 ABL E I (130) ER NA 2&5 0 24 WS 11/05/58 138 ER 5 1 0 25 PIONEER-II 11/08/58 ABL E I (129) ER 4 3 0 26 WS . 11/26 /58 140 ER 5 1 0 27 WS 12/05/58 145 ER 4 1 0 28 WS 12/16 /58 146 ER 4 1 0 29 WS 12/30/58 149 ER 2 1 0 30 WS 01/23/59 ABLE 11(128) ER 4 1.5 0 31 WS 01/30/59 154 ER 4 1 0 32 WS 02/28/59 ABL E II (131) ER 4 2 0 33 WS 03/21/59 ABL E II (132) ER 0 34 WS 03/21/59 158 ER 0 35 WS 03/26 /59 16 2 ER 0 36 WS 04/07/59 ABL E II (133) ER 0 37 WS 04/22/59 176 ER 0 38 WS 04/24/59 16 4 ER 0 39 WS 05/12/59 187 ER 0 40 WS 05/21/59 ABL E II (135) ER 0 41 WS 05/22/59 184 ER 0 9/10/96 165 RTI No. Mission/ID L aunch D ate Vehicle Configuration Test Range Response Mode Flight Phase Rep. Conf. 42 ws 06 /11/59 ABLE II (137) ER 0 43 WS 06 /25/59 198 ER 0 44 WS 06 /29/59 194 ER NA 1.5 0 45 WS 07/21/59 203 ER 3 1 0 46 WS 07/24/59 202 ER 0 47 WS 08/05/59 208 ER 0 48 EXPL ORER 6 08/07/59 ABLE III (134) ER 0 49 WS 08/14/59 204 ER 0 50 WS 08/27/59 216 ER 0 51 WS 09/12/59 217 ER 0 52 TRANSIT 1A 09/17/59 ABLE (136 ) ER 4 2.5 0 53 WS 09/22/59 222 ER 0 54 WS 10/06 /59 235 ER 0 55 WS 10/13/59 221 ER 0 56 WS 10/28/59 230 ER 0 57 WS 11/03/59 238 ER 0 58 WS 11/19/59 244 ER 0 59 WS 12/01/59 254 ER 4T 1 0 6 0 WS 12/17/59 255 ER 0 6 1 WS 01/14/6 0 256 ER 0 6 2 WS 02/09/6 0 259 ER 0 6 3 WS 02/29/6 0 26 3 ER 0 6 4 PIONEER-5 03/11/6 0 ABL E (219) ER 0 6 5 TIROS 1 04/01/6 0 ABL E (148) ER 0 6 6 TRANSIT-1 B 04/13/6 0 ABLE-STAR (257) ER NA 1 &5 0 6 7 TRANSIT-2A 06 /22/6 0 ABLE-STAR (281) ER NA 2&5 0 6 8 COURIER-1A 08/18/6 0 ABL E-STAR (26 2) ER 4T 1 0 6 9 COURIER-1 B 10/04/6 0 ABL E-STAR (293) ER 0 70 TRANSIT-3A 11/30/6 0 ABL E-STAR (283) ER 4 1 0 71 TRANSIT-3B 02/21/6 1 ABLE-STAR (313) ER NA 4&5 0 72 TRANSIT-4A 06 /28/6 1 ABLE-STAR (315) ER 0 73 TRANSIT-4B 11/15/6 1 ABLE-STAR (305) ER 0 74 BIG SH OT-1 (sub-orb.) 01/15/6 2 337 ER 0 75 COMPOSITE-1 01/24/6 2 ABL E-STAR (311) ER 5 2 0 76 WS 05/02/6 2 177 ER 0 77 ANNA-1A 05/10/6 2 ABLE-STAR (314) ER 4 2 0 78 BIG SH OT-II (sub-orb.) 07/18/6 2 338 ER 0 79 ANNA-1 B 10/31/6 2 ABL E-STAR (319) ER 0 80 ASSET ASV-1 09/18/6 3 232 ER 0 81 ASSET ASV-2 03/24/6 4 240 ER 4 2 0 82 ASSET ASV-3 07/22/6 4 250 ER 0 83 ASSET AEV-1 10/27/6 4 26 0 ER 0 84 ASSET AEV-2 12/08/6 4 SL VII (247) ER 0 85 ASSET ASV-4 02/23/6 5 248 ER 0 9/10/96 166 RTI D .5.2 Thor and Thor-Boosted Failure Narratives The following narratives provide information about flight failure of Thor weapons system and Thor-boosted space vehicle launches beginning with the first Thor launch in January 1957. The narratives are numbered to match the flight-sequence numbers in Section D .5.1. 1. 101, 25 Jan 57, Response M ode 1, Flight Phase 1: Failure of fuel-system valve resulted in loss of thrust. M issile fell back on pad after reaching an altitude of only 9 inches. 2. 102, 19 A pr 57, Response M ode 4, Flight Phase 1: M issile was apparently performing normally until destroyed by the RSO at 34.7 seconds. Erroneous D OVA P beat-beat plot showed missile heading uprange. 3. 103, 21 M ay 57, Response M ode 1, Flight Phase 1: M issile was destroyed on the pad at T - 5 minutes. A faulty fuel-tank regulator and relief valve resulted in over-pressurizing and bursting of fuel tank. 4. 104, 30 A ug 57, Response M ode 4T, Flight Phase 1: Spurious signals in the main- engine yaw feedback circuit resulted in missile breakup shortly after 92 seconds. 5. 105,20 Sep 57, Response M ode 4, Flight Phase 1: Premature propellant depletion resulted in impact some 400 miles short of target. 6. 107, 3 Oct 57, Response M ode 1, Flight Phase 1: M ain fuel valve closed 1.25 seconds after liftoff. M issile fell back on pad after reaching an altitude of about 17 feet. 7. 108,11 Oct 57, Response M ode 4, Flight Phase 1: D ue to a mechanical failure, an abnormal main-engine shutdown (one second early) resulted in loss of the vernier solo phase. 9. 112,7 D ec 57, Response M ode 5, Flight Phase 1: A n electrical-system failure at 107 seconds produced an abnormal loading on the missile converter. The missile began deviating at 110 seconds and finally broke up at about 224 seconds (well after M EC O at 156 seconds). M issile impacted 200 miles downrange and 40 miles left of flight line. 10. 113, 19 D ec 57, Response M ode 4, Flight Phase 1.5: Flight was regarded as successful although there was no vernier solo operation and impact was 6 miles from target. 11. 114, 28 Jan 58, Response M ode 5, Flight Phase 1: G uidance system failure at 95 seconds resulted in erroneous steering commands causing the vehicle to yaw left and pitch down. D ivergence began about 110 seconds and continued until the 9/10/96 167 RTI vehicle was destroyed by the RSO at 152 seconds. M issile impacted about 60 miles downrange. 12. 120, 28 Feb 58, Response M ode 4, Flight Phase 1: Failure of fuel line caused premature main engine shutdown at 109.7 seconds. 13. 121,19 A pr 58, Response M ode 1, Flight Phase 1: Failure of fuel system resulted in loss of thrust shortly after liftoff. M issile fell back on pad after reaching an altitude of about 4 feet. 14. 116 (A ble I), 23 A pr 58, Response M ode 4, Flight Phase 1: A turbopump failure at 146.2 seconds resulted in main-engine shutdown and an explosion. 18. 123, 11 July 58, Response M ode 4, Flight Phase 1: A lthough the flight was regarded as a success, the main engine failed to respond to the guidance shutdown command due to a wiring failure. W hen the main engine was shut down 0.43 seconds later by a backup command, the vernier engines also shut down. A large overshoot resulted from the late shutdown. 20. 126, 26 July 58, Response M ode 4, Flight Phase 1: A n inadvertent closing of the main-engine liquid-oxygen valve terminated thrust at 58.4 seconds. M issile components were recovered about 5 miles downrange. 22. 127 (A ble I), 17 A ug 58, Response M ode 4, Flight Phase 1: A turbopump failure led to main engine shutdown at about 74 seconds. A n explosion followed with impact about 10 miles downrange. 23. 130 (Pioneer I), 11 Oct 58, Response M ode NA , Flight Phase 2 & 5: Low upper­ stage thrust reduced the planned orbital altitude from 250,000 nm to 90,000 nm. 24. 138, 5 Nov 58, Response M ode 5, Flight Phase 1: Shortly after liftoff the missile began drifting uprange and to the left, reaching a maximum uprange drift of 150 feet. It continued diverging to the left of the nominal flight path until a pitch-gyro failure caused an excessive pitch down. Shortly thereafter at 34.6 seconds, command destruct occurred. 25. 129 (A ble I), 8 Nov 58, Response M ode 4, Flight Phase 3: A fter a normal boost phase, the third-stage (A llegheny Ballistic X-248-A 3) solid-propellant motor failed to ignite. 26. 140, 26 Nov 58, Response M ode 5, Flight Phase 1: Erratic performance of the guidance-system inverter at 111.4 seconds resulted in erroneous accelerometer scale factors and a 37 mile overshoot of target. Flight was regarded as a success. 27. 145, 5 D ec 58, Response M ode 4, Flight Phase 1: A lthough the flight was considered successful, below-normal thrust throughout flight resulted in fuel 9/10/96 168 RTI depletion before to reaching cutoff conditions. Impact was 28 miles short of target. 28. 146,16 D ec 58, Response M ode 4, Flight Phase 1: A lthough flight was considered a success, the main-engine fuel valve remained partially open for 14 seconds after M EC O command was given. This resulted in a 6-mile overshoot. 29. 149, 30 D ec 58, Response M ode 2, Flight Phase 1: A momentary ground in the electrical system at liftoff caused the guidance system to assume control at this time rather than the planned 108.5 seconds. G uidance immediately commanded a maximum pitch rate to place the missile in its proper orientation for 108.5 seconds. By 22 seconds the missile has pitched through 46°. A s it attempted to maintain stability, a reverse pitch subsequently developed, but by 46.4 seconds the missile was tumbling to the right. D estruct was sent at 52.5 seconds. 30. 128 (A ble II), 22 Jan 59, Response M ode 4, Flight Phase 1.5: A n electrical failure prevented second-stage (A erojet G eneral A J10-42) separation and ignition. 31. 154,30 Jan 59, Response M ode 4, Flight Phase 1: Improper propellant mixture and low thrust resulted in fuel depletion before cutoff conditions were reached. 32. 131 (A ble II), 28 Feb 59, Response M ode 4, Flight Phase 2: Flight appeared normal until 195 seconds when all track was lost. A s a result, the RSO sent cutoff at 218 seconds and destruct at 222 seconds. 44. 194, 29 June 59, Response M ode NA , Flight Phase 1.5: Flight was normal except that reentry vehicle did not separate and retro rockets did not fire. 45. 203,21 July 59, Response M ode 3, Flight Phase 1: The liftoff pin failed to extract so the pitch and roll programs were not initiated. M issile was destroyed at 45 seconds at an altitude of about 18,000 feet. 52. 136 (Transit 1A ), 17 Sep 59, Response M ode 4, Flight Phase 2.5: First and second stages performed normally until stage 2/3 separation. Failure of the stage-2 retro system apparently led to a collision of the stages. A s a result, the third stage failed to ignite. 59. 254, 1 D ec 59, Response M ode 4T, Flight Phase 1: A hydraulic-system failure resulted in premature closure of the main-engine liquid-oxygen valve. The hydraulic-system pressure decayed almost linearly from 8 seconds to 146 seconds when missile control was lost. Impact was 322 miles short of target. 66. 257 (Transit IB), 13 A pr 60, Response M ode NA , Flight Phase 1 and 5: The flight was a partial success although satellite was placed in a lower-than-planned orbit. M EC O velocity was 315 ft/sec below normal. Noisy data rejected by the guidance computer resulted in pitch-plane steering errors and the unplanned orbit. 9/10/96 169 RTI 67. 281 (Transit 2A ), 22 June 60, Response M ode NA , Flight Phase 2 and 5: A lthough boost phase was normal, anomalous performance during second-stage burn produced an orbit with apogee of 570 miles and perigee of 341 miles instead of the planned 500-mile circular orbit. 68. 262 (C ourier 1A ), 18 A ug 60, Response M ode 4T, Flight Phase 1: H ydraulic pressure began a steady decay beginning about 18 seconds after liftoff. Severe transients were noted at 129.3 seconds. U ncontrolled yaw, pitch, and roll maneuvers began about 133 seconds. Between 138 and 143 seconds the missile turned through three full revolutions in pitch. The upper stages separated at 140.4 seconds and the first stage broke up about 142.8 seconds. The second stage remained intact and was beacon tracked until 400 seconds. 70. 283 (Transit 3A ), 30 Nov 60, Response M ode 4, Flight Phase 1: The first stage shut down 11.2 seconds prematurely at 151.85 seconds when the M EC O cutoff circuit was armed. Since velocity at that time was about 2500 ft/sec below the normal cutoff velocity, portions of the first stage impacted in C uba. The second stage separated and performed normally until shut down by the RSO at M EC O plus 159.9 seconds to prevent overflight of South A merica. 71. 313 (Transit 3B), 21 Feb 61, Response M ode NA , Flight Phase 4 and 5: Second bum of second stage failed to occur. This resulted in an orbit with perigee of 539 miles and apogee of 92 miles instead of the planned 500-mile circular orbit. 75. 311 (C omposite I), 24 Jan 62, Response M ode 5, Flight Phase 2: Flight was within acceptable limits until second-stage ignition. Probably because of rupture of the lower oxidizer manifold, normal thrust levels never developed. A bout 50 milliseconds after ignition, severe thrust chamber motion developed and the second stage began to tumble. Telemetry indicated that the first tumble period was about 29 seconds. Propellant depletion occurred at M EC O plus 212 seconds. The nominal first-bum duration was 378 seconds. 77. 314 (A NNA 1A ), 10 M ay 62, Response M ode 4, Flight Phase 2: A fter a successful Thor flight, an electrical malfunction prevented separation and second-stage ignition. 81. 240 (A sset-2), 24 M ar 64, Response M ode 4, Flight Phase 2: The second stage either failed to ignite or burned for only one second. 9/10/96 170 RTI References 1. M ontgomery, R. M ., and W ard, J. A ., "C omputations of H it Probabilities From Launch-Vehicle D ebris", RTI/4666/02F, September 19,1990. 2. Eastern Test Range D irectorate of Safety Post-Test Report, Test D 1000,18 June 1991. 3. W ard, James A ., "Baseline Launch-A rea Risks for A tlas and D elta Launches", RTI/5180/60/40F, September 30,1995. 4. "Spacelift Effective C apacity: Part 1 - Launch Vehicle Projected Success Rate A nalysis", D raft, Booz«A llen & H amilton, Inc., 19 February 1992, prepared for the A ir Force Space C ommand Launch Services Office. 5. "Launch Options for the Future: Special Report", Office of Technology A ssessment, July 1988. 6. Silke, K evin, "Reliability G rowth M odel Overview", G eneral D ynamics Reliability Bulletin 92-02. 7. "Eastern Range Launches, 1950 - 1954, C hronological Summary", 45th Space W ing H istory Office. 8. "Eastern Range Launches, C hronological Summary", 45th Space W ing H istory Office, Extension updating the launch summary through 30 D ecember 1995. 9. "Vandenberg A FB Launch Summary", H eadquarters 30th Space W ing, Office of H istory, Launch C hronology, 1958 -1995. 10. Isakowitz, Steven J., (updated by Jeff Samella), International Reference Guide to Space Launch Systems, Second Edition, published and distributed by A IA A in 1995. 11. Smith, O. G ., "Launch Systems for M anned Spacecraft", D raft, July 23,1991. 12. "C omparison of Orbit Parameters - Table 1", prepared by M cD onnell D ouglas Space Systems C ompany, D elta launches through 4 Nov 95. 13. M issiles/Space Vehicle Files, 45th Space W ing, W ing Safety, M ission Flight C ontrol and A nalysis (SEO), 1957 through 1995. 14. M issile Launch Operations Logs, 30th Space W ing, copies provided via A C TA , Inc., (M r. James Baeker), 1963 through 1995. 9/10/96 171 RTI 15. "Titan IV, A merica's Silent H ero", published by Lockheed M artin in Florida Today, 13 Nov 95. 16. "A tlas Program Flight H istory" (through A pril 1965), G eneral D ynamics Report EM -1860,26 A pril 1965. 17. Fenske, C . W ., "A tlas Flight Program Summary", Lockheed M artin, A pril 1995. 18. Brater, Bob, "Launch H istory", Lockheed M artin FA X to* RTI, M arch 13,1996. 19. Several U SA F A ccident/Incident Reports for A tlas and Titan failures. 20. Quintero, A ndrew H ., "Launch Failures from the Eastern Range Since 1975", A erospace memo, February 25,1996, provided to RTI by Bill Zelinsky. 21. Set of "Titan Flight A nomaly/Failure Summary" since 1959, received from Lockheed M artin, A pril 4,1996. 22. C hang, I-Shih, "Space Launch Vehicle Failures (1984 - 1995)", A erospace Report No. TOR-96(8504)-2, January 1996. 9/10/96 172 RTI