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 |