Genesis will be the first mission to return samples from beyond the Earth-Moon system. The spacecraft will be inserted into a halo orbit about the L1 (Sun-Earth) libration point where it will remain for two years collecting solar wind particles. Upon Earth return, the sample return capsule, which is passively controlled, will descend under parachute to Utah. The present study describes the analysis of the entry, descent, and landing scenario of the returning sample capsule. The robustness of the entry sequence is assessed through a Monte Carlo dispersion analysis where the impact of off-nominal conditions is ascertained. The dispersion results indicate that the capsule attitude excursions near peak heating and drogue chute deployment are within Genesis mission limits. Additionally, the size of the resulting 3-sigma landing ellipse is 47.8 km in downrange by 15.2 km in crossrange, which is within the Utah Test and Training Range boundaries.
Entry Dispersion Analysis for the Genesis Sample Return Capsule
AAS/AIAA Astrodynamics Specialists Conference ; 1999 ; Girdwood, AK, United States
2005-01-01
Preprint
No indication
English
FULL, LENGTH PAPERS - Entry Dispersion Analysis for the Genesis Sample Return Capsule
Online Contents | 2001
|Entry Dispersion Analysis for the Genesis Sample Return Capsule (AAS 99-469)
British Library Conference Proceedings | 2000
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