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Distinctive Carbonates in Five Martian Meteorites: Search for Water on MarsRecently published results from Mars orbital data strongly support both the idea that large bodies of water were present at the surface in the past and the possibility that significant amounts of water ice are currently present in the regolith just below the planet's surface. These new findings increase the significance of the evidence in martian meteorites that some low-temperature aqueous alteration and secondary mineral deposition occurred on Mars.
Document ID
20050199283
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
Wentworth, Susan J.
(Lockheed Martin Corp. Houston, TX, United States)
Bailey, Jake
(NASA Johnson Space Center Houston, TX, United States)
McKay, David S.
(NASA Johnson Space Center Houston, TX, United States)
Thomas-Keprta, Kathie L.
(Lockheed Martin Corp. Houston, TX, United States)
Velbel, Michael
(Michigan State Univ. East Lansing, MI, United States)
Date Acquired
August 23, 2013
Publication Date
January 1, 2003
Publication Information
Publication: Living Links Through Time and Space: Meeting the Challenges of Interdisciplinary Science
Subject Category
Lunar And Planetary Science And Exploration
Report/Patent Number
JSC-CN-7745
Paper 12639
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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