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The evolution of CO2 on MarsAt the surface, the atmosphere of Mars contains approximately 95.3 percent CO2 by volume. At the Viking Lander 1 (VL1) site, the total surface pressure varied with the season between about 6.89 and 8.94 mbar. Questions related to the observed CO2 pressure on Mars are explored. Several published estimates of the total amount of CO2 outgassed over the history of Mars, varying between 140 and 3000 mbar, are shown in a table. It is pointed out that the study of likely reservoirs for outgassed CO2 has focused mainly on the polar caps and regolith. Constraints on the formation of transitory pockets of moist soil are discussed, taking into account heat requirements, supply of water, and constraints related to pressure. Attention is also given to chemical considerations, implications for the current status of CO2 reservoirs, and scenarios for the evolution of CO2 pressure.
Document ID
19850056130
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Kahn, R.
(Washington University St. Louis, MO; Cornell University, Ithaca, NY, United States)
Date Acquired
August 12, 2013
Publication Date
May 1, 1985
Publication Information
Publication: Icarus
Volume: 62
ISSN: 0019-1035
Subject Category
Lunar And Planetary Exploration
Report/Patent Number
ISSN: 0019-1035
Accession Number
85A38281
Funding Number(s)
CONTRACT_GRANT: NAGW-660
CONTRACT_GRANT: NSG-6612
Distribution Limits
Public
Copyright
Other

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