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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Bibliographic Details
Main Authors: Clark, B. C., Baird, A. K.
Format: Other/Unknown Material
Language:unknown
Published: 1979
Subjects:
91
Ice
Online Access:http://ntrs.nasa.gov/search.jsp?R=19800026295
id ftnasantrs:oai:casi.ntrs.nasa.gov:19800026295
record_format openpolar
spelling 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)
institution Open Polar
collection NASA Technical Reports Server (NTRS)
op_collection_id ftnasantrs
language 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
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