Volatiles in the Martian regolith
An inventory of released volatiles on Mars has been derived based upon Viking measurements of atmospheric and surface chemical composition, and upon the inferred mineralogy of a ubiquitous regolith, assumed to average 200m in depth. This model is consistent with the relative abundances of volatiles...
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ftnasantrs:oai:casi.ntrs.nasa.gov:19800026295 2023-05-15T16:37:28+02:00 Volatiles in the Martian regolith Clark, B. C. Baird, A. K. Unclassified, Unlimited, Publicly available Oct 1, 1979 http://ntrs.nasa.gov/search.jsp?R=19800026295 unknown http://ntrs.nasa.gov/search.jsp?R=19800026295 Accession ID: 80A10465 Copyright Other Sources 91 Geophysical Research Letters; 6; Oct. 197 1979 ftnasantrs 2012-02-15T14:15:35Z An inventory of released volatiles on Mars has been derived based upon Viking measurements of atmospheric and surface chemical composition, and upon the inferred mineralogy of a ubiquitous regolith, assumed to average 200m in depth. This model is consistent with the relative abundances of volatiles (except for S) on the earth's surface, but implies one-fifteenth of the volatile release of earth if starting materials were comparable. All constituents are accommodated as chemical components of, or absorbed phases on, regolith materials - without the necessity of invoking unobservable deposits of carbonates, nitrates, or permafrost ice. Other/Unknown Material Ice permafrost NASA Technical Reports Server (NTRS) |
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NASA Technical Reports Server (NTRS) |
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ftnasantrs |
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unknown |
topic |
91 |
spellingShingle |
91 Clark, B. C. Baird, A. K. Volatiles in the Martian regolith |
topic_facet |
91 |
description |
An inventory of released volatiles on Mars has been derived based upon Viking measurements of atmospheric and surface chemical composition, and upon the inferred mineralogy of a ubiquitous regolith, assumed to average 200m in depth. This model is consistent with the relative abundances of volatiles (except for S) on the earth's surface, but implies one-fifteenth of the volatile release of earth if starting materials were comparable. All constituents are accommodated as chemical components of, or absorbed phases on, regolith materials - without the necessity of invoking unobservable deposits of carbonates, nitrates, or permafrost ice. |
format |
Other/Unknown Material |
author |
Clark, B. C. Baird, A. K. |
author_facet |
Clark, B. C. Baird, A. K. |
author_sort |
Clark, B. C. |
title |
Volatiles in the Martian regolith |
title_short |
Volatiles in the Martian regolith |
title_full |
Volatiles in the Martian regolith |
title_fullStr |
Volatiles in the Martian regolith |
title_full_unstemmed |
Volatiles in the Martian regolith |
title_sort |
volatiles in the martian regolith |
publishDate |
1979 |
url |
http://ntrs.nasa.gov/search.jsp?R=19800026295 |
op_coverage |
Unclassified, Unlimited, Publicly available |
genre |
Ice permafrost |
genre_facet |
Ice permafrost |
op_source |
Other Sources |
op_relation |
http://ntrs.nasa.gov/search.jsp?R=19800026295 Accession ID: 80A10465 |
op_rights |
Copyright |
_version_ |
1766027767323820032 |