Rare gases in the atmospheres of Venus, earth, and Mars and the problem of the origin of planetary atmospheres

Details Rare gases in the atmospheres of Venus, earth, and Mars and the problem of the origin of planetary atmospheres Rare gases in the atmospheres of Venus, earth, and Mars and the problem of the origin of planetary atmospheres

Jul 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979kosis..17..602i&link_type=abstract

Kosmicheskie Issledovaniia, vol. 17, July-Aug. 1979, p. 602-610. In Russian.

Computer Science

1

Atmospheric Composition, Earth Atmosphere, Planetary Evolution, Rare Gases, Venus Atmosphere, Hypotheses

Scientific paper

Data on rare gas concentrations in the atmospheres of earth, Mars, and Venus lead to the suggestion that the atmospheres of these planets were created by gas accretion from the solar nebula. This primary gaseous component was supplemented by a secondary component produced by degasing of the lithosphere. The proposed hypothesis allows a simpler explanation of certain features of planetary formation than does the secondary-atmosphere theory.

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