Possible Mafic Patches in Scott Crater Highlight the Need for Resource Exploration on the Lunar South Polar Region
Possible areas of mafic material on the rim and floor of Scott crater (82.1 deg S, 48.5 deg E) are suggested by analysis of shadow-masked Clementine false-color-ratio images. Mafic materials common in mare and pyroclastic materials can produce more oxygen than can highlands materials, and mafic mate...
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2007
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ftnasantrs:oai:casi.ntrs.nasa.gov:20070014474 2023-05-15T18:22:11+02:00 Possible Mafic Patches in Scott Crater Highlight the Need for Resource Exploration on the Lunar South Polar Region Cooper, Bonnie L. Unclassified, Unlimited, Publicly available [2007] application/pdf http://hdl.handle.net/2060/20070014474 unknown Document ID: 20070014474 http://hdl.handle.net/2060/20070014474 No Copyright CASI Lunar and Planetary Science and Exploration Lunar Reconnaissance Orbiter High Resolution Image; 3-5 May 2007; Houston, TX; United States 2007 ftnasantrs 2019-07-21T01:41:00Z Possible areas of mafic material on the rim and floor of Scott crater (82.1 deg S, 48.5 deg E) are suggested by analysis of shadow-masked Clementine false-color-ratio images. Mafic materials common in mare and pyroclastic materials can produce more oxygen than can highlands materials, and mafic materials close to the south pole may be important for propellant production for a future lunar mission. If the dark patches are confirmed as mafic materials, this finding would suggest that other mafic patches may exist, even closer to the poles, which were originally mapped as purely anorthositic. Other/Unknown Material South pole NASA Technical Reports Server (NTRS) South Pole |
institution |
Open Polar |
collection |
NASA Technical Reports Server (NTRS) |
op_collection_id |
ftnasantrs |
language |
unknown |
topic |
Lunar and Planetary Science and Exploration |
spellingShingle |
Lunar and Planetary Science and Exploration Cooper, Bonnie L. Possible Mafic Patches in Scott Crater Highlight the Need for Resource Exploration on the Lunar South Polar Region |
topic_facet |
Lunar and Planetary Science and Exploration |
description |
Possible areas of mafic material on the rim and floor of Scott crater (82.1 deg S, 48.5 deg E) are suggested by analysis of shadow-masked Clementine false-color-ratio images. Mafic materials common in mare and pyroclastic materials can produce more oxygen than can highlands materials, and mafic materials close to the south pole may be important for propellant production for a future lunar mission. If the dark patches are confirmed as mafic materials, this finding would suggest that other mafic patches may exist, even closer to the poles, which were originally mapped as purely anorthositic. |
format |
Other/Unknown Material |
author |
Cooper, Bonnie L. |
author_facet |
Cooper, Bonnie L. |
author_sort |
Cooper, Bonnie L. |
title |
Possible Mafic Patches in Scott Crater Highlight the Need for Resource Exploration on the Lunar South Polar Region |
title_short |
Possible Mafic Patches in Scott Crater Highlight the Need for Resource Exploration on the Lunar South Polar Region |
title_full |
Possible Mafic Patches in Scott Crater Highlight the Need for Resource Exploration on the Lunar South Polar Region |
title_fullStr |
Possible Mafic Patches in Scott Crater Highlight the Need for Resource Exploration on the Lunar South Polar Region |
title_full_unstemmed |
Possible Mafic Patches in Scott Crater Highlight the Need for Resource Exploration on the Lunar South Polar Region |
title_sort |
possible mafic patches in scott crater highlight the need for resource exploration on the lunar south polar region |
publishDate |
2007 |
url |
http://hdl.handle.net/2060/20070014474 |
op_coverage |
Unclassified, Unlimited, Publicly available |
geographic |
South Pole |
geographic_facet |
South Pole |
genre |
South pole |
genre_facet |
South pole |
op_source |
CASI |
op_relation |
Document ID: 20070014474 http://hdl.handle.net/2060/20070014474 |
op_rights |
No Copyright |
_version_ |
1766201554075910144 |