Venus Entry Options Venus Upper Atmosphere Investigations Science and Technical Interchange Meeting (STIM)

Transcription

1 Venus Entry Options Venus Upper Atmosphere Investigations Science and Technical Interchange Meeting (STIM) January 24, 2013 at the Ohio Aerospace Institute Peter Gage, Gary Allen, Dinesh Prabhu, Ethiraj Venkatapathy 1

2 Characteristics of the Entry Problem Entry velocity Driven by interplanetary trajectory Entry angle Must be high enough to avoid skip-out Affects latitude that can be reached Ballistic coefficient Design choice, constrained by packaging Heating rate Constrains material selection Heat load Drives thermal protection thickness Deceleration Drives payload structural requirements ADEPT/NASA Distribution Only 2

3 TPS Mass Scales with Heat Load From Laub and Venkatapathy September 14, 2012 ADEPT/NASA Distribution Only 3

4 Entry Environments for Previous Missions b = 600 Venera 4, 5, 6 Venera/Vega P-V Large Probe September 14, 2012 ADEPT/NASA Distribution Only 4

5 Entry Performance Entry Vehicle Class Ballistic Coefficient Entry Angle Peak deceleration (g s) Peak heat flux (kw/cm2) Total heat load (kj/cm2) Venera >23 Vega Pioneer Large TPS mass fraction (%) ADEPT ~12 (estimated) All cases assume V=11.2 km/s Cases are representative, not matching actual mission conditions September 14, 2012 ADEPT/NASA Distribution Only 5

6 Altitude (km) Venus Entry: Time to Mach ADEPT Pioneer Large Vega Venera Time (s) ADEPT/NASA Distribution Only 6

7 Adaptive Deployable Entry and Placement Technology ADEPT-VITaL Key Facts Launch Vehicle Atlas V 551 Launch Date 29 May 2023 Entry Date 29 September 2024 Entry Flight Path Angle -8.25º Atlas V 551 Launch ADEPT remains stowed during Interplanetary cruise; Deployment at Venus Entry Velocity 10.8 km/s Entry Azimuth Angle 171.0º Peak G-load (nominal) Peak G-load (3s) 30 G 46 G Ballistic Entry (unguided) 6-m Diameter 70º Cone Subsonic parachute for ADEPT separation and VITaL Lander release Landing in Alpha region Alpha Landing Ellipse Estimated 600 km x 600 km 3s landing location uncertainty ellipse based on 2000 case POSTII Monte Carlo with uncertainties in: Entry Position, Entry FPA, Entry Velocity, Drag Coefficient, Density, Wind May 15, 2012 ADEPT/CA250/NASA Distribution Only 7

8 Altitude (km) Any benefit from lifting entry? L/D=0.2 L/D=0 Targeting accuracy Cross range Time Ballistic Coefficient Entry Angle Peak deceleration (g s) Peak heat flux (kw/cm2) Total heat load (kj/cm2) ADEPT Ballistic ADEPT L/D= September 14, 2012 ADEPT/NASA Distribution Only 8

9 Deployment Environment: Venus and Mars UAV design experience from Mars may be relevant for Venus September 14, 2012 ADEPT/NASA Distribution Only 9

10 Summary Vega provides existence proof for entry capability for balloons Requires Carbon Phenolic or equivalent More mass efficient solutions are available Pioneer Venus has similar altitude for M=1 More mass efficient, higher peak deceleration ADEPT decelerates higher, with much lower peak deceleration Opportunity for unfolding UAVs Technology development is in progress Lifting entry adds complexity without obvious benefit September 14, 2012 ADEPT/NASA Distribution Only 10

11 BACKUP September 14, 2012 ADEPT/NASA Distribution Only 11

12 Engineering Challenges for High-Speed Atmospheric Entry Venus Example For rigid aeroshell Size constrained by launch shroud Entry mass constrained by launch vehicle throw capability Ballistic coefficient ~ 250 kg/m 2 Need material that can sustain 2000 W/cm2 Only Carbon Phenolic is available 9/14/

13 Engineering Challenges for High-Speed Atmospheric Entry Venus Example For rigid aeroshell Size constrained by launch shroud Entry mass constrained by launch vehicle throw capability Ballistic coefficient ~ 250 kg/m 2 For a given material, operating near its heating rate capability reduces heat load, which reduces TPS mass 9/14/

14 Engineering Challenges for High-Speed Atmospheric Entry Venus Example For rigid aeroshell Size constrained by launch shroud Entry mass constrained by launch vehicle throw capability Ballistic coefficient ~ 250 kg/m 2 Select entry angle with favorable balance of heat rate and heat load Accept high deceleration (250 g) Certify for this load environment 9/14/

15 Opportunity for High-Speed Atmospheric Entry Venus Example Operate at a lower ballistic coefficient Develop a lower-density material that can sustain 2000 W/cm2 9/14/

16 Opportunity for High-Speed Atmospheric Entry Venus Example Assume ballistic coefficient can be lowered 10 x A material that can sustain 200 W/cm2 is now feasible Peak deceleration reduced by an order of magnitude 9/14/