Distribution of water on Mars: Implications from SNC meteorites

There has been much speculation about the abundance of water and other volatiles on Mars. Attempts to calculate abundances of water on Mars indicate that Mars contains approx. 10-100 m of water. Numerous models have been put forth to determine the amount of water on Mars more closely. Some researche...

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Main Author: Jones, J. H.
Format: Other/Unknown Material
Language:unknown
Published: 1992
Subjects:
91
Online Access:http://ntrs.nasa.gov/search.jsp?R=19920019784
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spelling ftnasantrs:oai:casi.ntrs.nasa.gov:19920019784 2023-05-15T17:57:36+02:00 Distribution of water on Mars: Implications from SNC meteorites Jones, J. H. Unclassified, Unlimited, Publicly available JAN 1, 1992 http://ntrs.nasa.gov/search.jsp?R=19920019784 unknown http://ntrs.nasa.gov/search.jsp?R=19920019784 Accession ID: 92N29027 No Copyright CASI 91 Lunar and Planetary Inst., Workshop on the Martian Surface and Atmosphere Through Time; p 78-79 1992 ftnasantrs 2012-02-15T19:21:29Z There has been much speculation about the abundance of water and other volatiles on Mars. Attempts to calculate abundances of water on Mars indicate that Mars contains approx. 10-100 m of water. Numerous models have been put forth to determine the amount of water on Mars more closely. Some researchers infer that Chassigny parent magma contained greater than 1.5 percent water by weight and that the Martian mantle contained greater than 1000 parts per million water. This is too much water for a depleted region. Perhaps some of the water in Chassigny was assimilated at shallow depths, either in a crustal magma chamber or by interaction with superficial permafrost. Either is possible and provides an alternative to the dilemma of water-rich to depleted regions. Other/Unknown Material 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
Jones, J. H.
Distribution of water on Mars: Implications from SNC meteorites
topic_facet 91
description There has been much speculation about the abundance of water and other volatiles on Mars. Attempts to calculate abundances of water on Mars indicate that Mars contains approx. 10-100 m of water. Numerous models have been put forth to determine the amount of water on Mars more closely. Some researchers infer that Chassigny parent magma contained greater than 1.5 percent water by weight and that the Martian mantle contained greater than 1000 parts per million water. This is too much water for a depleted region. Perhaps some of the water in Chassigny was assimilated at shallow depths, either in a crustal magma chamber or by interaction with superficial permafrost. Either is possible and provides an alternative to the dilemma of water-rich to depleted regions.
format Other/Unknown Material
author Jones, J. H.
author_facet Jones, J. H.
author_sort Jones, J. H.
title Distribution of water on Mars: Implications from SNC meteorites
title_short Distribution of water on Mars: Implications from SNC meteorites
title_full Distribution of water on Mars: Implications from SNC meteorites
title_fullStr Distribution of water on Mars: Implications from SNC meteorites
title_full_unstemmed Distribution of water on Mars: Implications from SNC meteorites
title_sort distribution of water on mars: implications from snc meteorites
publishDate 1992
url http://ntrs.nasa.gov/search.jsp?R=19920019784
op_coverage Unclassified, Unlimited, Publicly available
genre permafrost
genre_facet permafrost
op_source CASI
op_relation http://ntrs.nasa.gov/search.jsp?R=19920019784
Accession ID: 92N29027
op_rights No Copyright
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