Evolution of the atmospheres of the terrestrial planets

Details Evolution of the atmospheres of the terrestrial planets Evolution of the atmospheres of the terrestrial planets

Sep 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990avest..24..179c&link_type=abstract

Astronomicheskii Vestnik (ISSN 0320-930X), vol. 24, July-Sept. 1990, p. 179-194. In Russian.

Astronomy and Astrophysics

Astronomy

Atmospheric Composition, Climate Change, Earth Atmosphere, Mars Atmosphere, Planetary Atmospheres, Venus Atmosphere, Atmospheric Chemistry, Atmospheric Moisture, Carbon Dioxide Concentration, Clouds (Meteorology), Heavy Water

Scientific paper

It is pointed out that, even though the atmospheres of the earth, Venus, and Mars have distinctly different climates, it appears likely that all three planets were created under similar conditions; the planets are different only in terms of mass and incident solar radiation. This paper considers some of the difficulties in assessing the nature of the primordial climates and in extrapolating these climates to the present day. In particular, questions concerning clouds, water, and CO2 on the earth and on Mars are addressed.

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