The gas-surface interaction of a human-occupied spacecraft with a near-Earth object
W. M. Farrell, Dana M. Hurley, Michael J. Poston, Michael I. Zimmerman, Thomas M. Orlando, Charles A. Hibbitts, R. M. Killen
Abstract
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W. M. Farrell, Dana M. Hurley, Michael J. Poston, Michael I. Zimmerman, Thomas M. Orlando, Charles A. Hibbitts, R. M. Killen
Abstract
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NASA’s asteroid redirect mission (ARM) will feature an encounter of the human-occupied Orion spacecraft with a portion of a near-Earth asteroid (NEA) previously placed in orbit about the Moon by a capture spacecraft. Applying a shuttle analog, we suggest that the Orion spacecraft should have a dominant local water exosphere, and that molecules from this exosphere can adsorb onto the NEA. The amount of adsorbed water is a function of the defect content of the NEA surface, with retention of shuttle-like water levels on the asteroid at 1015 H2O’s/m2 for space weathered regolith at T ∼ 300 K.
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NASA’s asteroid redirect mission (ARM) will feature an encounter of the human-occupied Orion spacecraft with a portion of a near-Earth asteroid (NEA) previously placed in orbit about the Moon by a capture spacecraft. Applying a shuttle analog, we suggest that the Orion spacecraft should have a dominant local water exosphere, and that molecules from this exosphere can adsorb onto the NEA. The amount of adsorbed water is a function of the defect content of the NEA surface, with retention of shuttle-like water levels on the asteroid at 1015 H2O’s/m2 for space weathered regolith at T ∼ 300 K.
Key concepts: Spacecraft, Regolith, Exosphere, Astrobiology, Space weathering, Asteroid, Near-Earth object, Physics