Artemis III EVA Opportunities on the Lunar Farside near Shackleton Crater
Artemis III EVA Opportunities on the Lunar Farside near Shackleton Crater
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Date
2020-09-08
Authors
Kring, David A. (David Allen)
Bretzelder, Jordan M.
Ganesh, Indujaa
Kumari, Nandita
Lang, Antonio
https://orcid.org/0000-0002-3440-6282
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Abstract
A summit between Shackleton and Slater craters has an average solar illumination of 83%. The point, site 007 of [1] and NASA's Plan for Sustainable Lunar Exploration and Development, is on the farside of the Moon, beyond the south pole as seen from Earth (Fig. 1 & 2). Solar power at such sites may provide an important lunar surface resource if a distribution system can be developed. Adjacent to that point of illumination is a modest-size permanently shadowed region (PSR) in which water was detected from orbit [2]. Thus, the PSR may harbor icy regolith deposits, another resource, that may provide crew consumables, radiation shielding, and propellant.
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Moon--Exploration