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Artemis III EVA Mission Capability for de Gerlache-Shackleton RidgeNASA has committed to sending humans to the Moon no earlier than 2025. The Artemis III mission will include scientific, technology demonstrations, commercial, inspirational, and explorational objectives. Achieving these goals will depend upon balancing priorities and mission constraints. A landing location needs to meet terrain conditions suitable for the lander with acceptable thermal and lighting conditions. This location must also allow access to geological areas of interest within traverse range and capability of walking astronauts. A representative EVA timeline is then developed for an example location on the de Gerlache-Shackleton ridge and used to examine the location’s acceptability as a candidate site for Artemis III. Similar studies are being conducted to NASA’s Science Mission Directorate and Flight Operations.
Document ID
20210026296
Acquisition Source
Johnson Space Center
Document Type
Presentation
Authors
Zebulon C Scoville
(Johnson Space Center Houston, Texas, United States)
Date Acquired
January 3, 2022
Subject Category
Lunar And Planetary Science And Exploration
Meeting Information
Meeting: Lunar and Planetary Science Conference
Location: Woodlands, TX
Country: US
Start Date: March 7, 2022
End Date: March 11, 2022
Sponsors: Lunar and Planetary Institute
Funding Number(s)
WBS: 747797.07.01.10.01.01
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
Technical Review
Single Expert
Keywords
EVA
Lunar Geology
Artemis
PSR
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