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Stability of the Martian atmosphereA detailed chemical dynamic model is presented for a moist Martian atmosphere. Recombination of CO2 is catalyzed by trace amount of H2O. The abundances of CO and O2 should vary in response to changes in atmospheric H2O and atmospheric mixing.
Document ID
19730010098
Acquisition Source
Legacy CDMS
Document Type
Contractor Report (CR)
Authors
Mcelroy, M. B. (Harvard Univ. Cambridge, United States)
Donahue, T. M. (Pittsburgh Univ. Pittsburgh, PA, United States)
Date Acquired
September 2, 2013
Publication Date
August 1, 1972
Subject Category
Space Sciences
Report/Patent Number
NASA-CR-130799
SRCC-177
Accession Number
73N18825
Funding Number(s)
CONTRACT_GRANT: NGR-39-011-002
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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