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Entry Dispersion Analysis for the Genesis Sample Return Capsule
Author(s) -
Prasun N. Desai,
F. McNeil Cheatwood
Publication year - 2001
Publication title -
journal of spacecraft and rockets
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.758
H-Index - 79
eISSN - 1533-6794
pISSN - 0022-4650
DOI - 10.2514/2.3707
Subject(s) - spacecraft , aerospace engineering , missile , space (punctuation) , spacecraft design , systems engineering , space technology , dispersion (optics) , space exploration , space research , sample (material) , engineering , computer science , aeronautics , mechanical engineering , physics , operating system , optics , thermodynamics
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 anlaysis 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.

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