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Stability of the Martian Atmosphere

descriptionPublicationkeyboard_double_arrow_right Article 15 Sep 1972Publisher:American Association for the Advancement of Science (AAAS)Journal:Science, volume 177, pages 986-988 (issn: 0036-8075, eissn: 1095-9203,

Authors: Thomas M. Donahue; Michael B. McElroy;

doi: 10.1126/science.177.4053.986

pmid: 17788809

Stability of the Martian Atmosphere

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Abstract

A detailed chemical dynamic model is presented for a moist martian atmosphere. Recombination of carbon dioxide is catalyzed by trace amounts of water. The abundances of carbon monoxide and molecular oxygen should vary in response to changes in atmospheric water and atmospheric mixing.

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Harvard University
United States

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