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Artemis III EVA Opportunities on the Lunar Farside near Shackleton Crater

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dc.contributor.author Kring, David A. (David Allen)
dc.contributor.author Bretzelder, Jordan M.
dc.contributor.author Ganesh, Indujaa
dc.contributor.author Kumari, Nandita
dc.contributor.author Lang, Antonio
dc.contributor.author https://orcid.org/0000-0002-3440-6282
dc.coverage.spatial Moon
dc.date.accessioned 2020-10-30T17:03:32Z
dc.date.available 2020-10-30T17:03:32Z
dc.date.issued 2020-09-08
dc.identifier.uri https://hdl.handle.net/20.500.11753/1718
dc.description.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. en
dc.format.extent 2 pages
dc.format.mimetype application/pdf
dc.language.iso en en
dc.relation.ispartofseries LPI contribution ; no. 2565
dc.subject Moon--Exploration en
dc.title Artemis III EVA Opportunities on the Lunar Farside near Shackleton Crater en
dc.title.alternative Artemis 3 EVA Opportunities on the Lunar Farside near Shackleton Crater en
dc.type Working Paper en


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