Atmospheres as a clue to the early solar system

Details Atmospheres as a clue to the early solar system Atmospheres as a clue to the early solar system

Jul 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988rspta.325..569c&link_type=abstract

(Royal Society, Discussion on the Solar System: Chemistry as a Key to its Origin, London, England, July 15, 16, 1987) Royal Soci

Computer Science

2

Planetary Atmospheres, Solar System, Atmospheric Composition, Earth Atmosphere, Gas Giant Planets, Ice, Mars Atmosphere, Natural Satellites, Outgassing, Silicates

Scientific paper

Conditions that could have applied in the environments of the major planets when they were forming make it possible that the present icy mantles of the larger satellites were then oceans and vapour atmospheres encasing silicate-ferrous cores. The major constituents are explored by comparison with the present atmospheres of the terrestrial planets. It is further suggested that the primary condensations during the formation of the solar system were the Sun and the major planets, and that the terrestrial planets and satellites were a secondary formation. Some observational data are offered in support of the arguments and future tests are suggested.

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