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Artemis III EVA Opportunities on Malapert and Leibnitz β Massifs

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dc.contributor.author Kring, David A. (David Allen)
dc.contributor.author Gruener, John E.
dc.contributor.author Eppler, Dean B.
dc.coverage.spatial Moon
dc.date.accessioned 2020-10-28T20:00:39Z
dc.date.available 2020-10-28T20:00:39Z
dc.date.issued 2020-09-08
dc.identifier.uri https://hdl.handle.net/20.500.11753/1712
dc.description.abstract If Artemis III astronauts land on Malapert or Leibnitz β, the exploration and science rationales developed previously apply. If, however, they are limited to a 2 km walking EVA, the breadth of the science to be addressed will be considerably smaller. In the Constellation Lunar Surface Systems study, communication relay, solar power, and seismometer stations were to be deployed and a heat probe inserted into the regolith. The same can occur at an Artemis III landing site. en
dc.format.extent 2 pages
dc.format.mimetype application/pdf
dc.language.iso en en
dc.relation.ispartofseries LPI contribution ; no. 2559
dc.subject Moon--Exploration en
dc.title Artemis III EVA Opportunities on Malapert and Leibnitz β Massifs en
dc.title.alternative Artemis 3 EVA Opportunities on Malapert and Leibnitz Beta Massifs en
dc.type Working Paper en


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