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Wes Ousley June 28, 2001 SuperNova/ Acceleration Probe (SNAP) Thermal
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SNAP, June 25-28, 2001 Goddard Space Flight Center System Introduction Page 2 Overview Mission Requirements Selected Configuration and Rationale Mass, Power, and Cost Summary Risk Assessment Issues and Concerns Thermal Topics
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SNAP, June 25-28, 2001 Goddard Space Flight Center System Introduction Page 3 SNAP spacecraft thermal requirements can be accommodated with standard thermal control techniques (blankets, heaters, heat pipes) Spacecraft bus is thermally coupled to reduce eclipse cooldown Instrument CCD radiator should be moved to accommodate spacecraft radiator Thermal Overview
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SNAP, June 25-28, 2001 Goddard Space Flight Center System Introduction Page 4 High Earth orbit No significant albedo or earth IR Eclipse time (max 6 hours) drives bus thermal design CCD camera operates at 150K Passive radiator dissipates camera power and parasitic loads Thermal System Mission Requirements
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SNAP, June 25-28, 2001 Goddard Space Flight Center System Introduction Page 5 Spacecraft Thermal Configuration Bus thermal design radiates heat from anti-sun side Much smaller radiators than sun-side for same heat transfer Reduces eclipse heater power requirement Most internal bus components mounted to bottom deck Deck is honeycomb panel with imbedded heat pipes Thermal masses coupled to reduce eclipse cooldown Heat pipes transfer heat from deck to anti-sun radiator Prop system thermally isolated from deck Current configuration shows no anti-sun radiator margin! Restricting roll angle allows up to 200% size margin Moving CCD radiator permits 100% margin with +/-45 O roll
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SNAP, June 25-28, 2001 Goddard Space Flight Center System Introduction Page 6 Bus Layout Propulsion Tanks 5# thrusters (4 sets of 2) Sub-system electronics Anti-sun radiator
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SNAP, June 25-28, 2001 Goddard Space Flight Center System Introduction Page 7 Solar Array Thermal Configuration Solar array thermally isolated from telescope Telescope thermal stability is essential to mission success Array temperatures change significantly with pitch and roll angle Low-conductivity mounting and MLI behind array provide isolation Pitch of 30 O away from normal sun cools entire array by 10 O C With isolation, this lowers thermal environment inside baffle by less than 1% Roll angle of 45 O heats up sun-normal area by 30C, and cools opposite area by 100C Alters entire temperature field on secondary mirror structure Change in local environment input inside baffle up to 5%
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SNAP, June 25-28, 2001 Goddard Space Flight Center System Introduction Page 8 Telescope Configuration Propulsion Tanks Sub-system electronics Secondary Mirror and Mount Optical Bench Primary Mirror Thermal Radiator Solar Array Wrap around, body mounted 50% OSR & 50% Cells
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SNAP, June 25-28, 2001 Goddard Space Flight Center System Introduction Page 9 Telescope Thermal Configuration Baffle has MLI blankets on outside to reduce thermal swings MLI blankets between spacecraft and telescope optics volume Radiator of 2m 2 can remove 36W from 150K camera CCD radiator should be moved toward aperture to allow anti-sun area for spacecraft radiator
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SNAP, June 25-28, 2001 Goddard Space Flight Center System Introduction Page 10 Thermal Mass, Power, and Cost Summary Thermal system mass 67kg Heat pipes for deck and radiator 37kg MLI blankets on spacecraft total 28kg Heater power of 38W for prop thermal control Eclipse average heater power 40W Hardware cost is $910K Heat pipe panel cost $700K
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SNAP, June 25-28, 2001 Goddard Space Flight Center System Introduction Page 11 Thermal Risk Assessment Thermal design is low risk. Off-the-shelf hardware; custom designed heat pipe panels.
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SNAP, June 25-28, 2001 Goddard Space Flight Center System Introduction Page 12 Thermal Issues and Concerns 1. Allowed roll angle of 45 O causes substantial changes in secondary structure thermal environment 2. Relocation of CCD radiator is required to allow spacecraft radiator area if 45 O roll angle is baselined
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