Atmosphere-surface interactions on Venus and implications for atmospheric evolution

Details Atmosphere-surface interactions on Venus and implications for atmospheric evolution Atmosphere-surface interactions on Venus and implications for atmospheric evolution

Aug 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982p%26ss...30..803k&link_type=abstract

(IAU, IAMAP, and COSPAR, Joint Meeting on the Origin and Evolution of Planetary Atmospheres, Hamburg, West Germany, Aug. 17, 18,

Physics

8

Air Land Interactions, Atmospheric Composition, Planetary Evolution, Venus Atmosphere, Venus Surface, Chemical Composition, Chemical Evolution, Chemical Reactions, Pioneer Venus Spacecraft, Planetary Composition, Planetary Crusts, Surface Properties, Troposphere, Venera 11 Satellite

Scientific paper

The physicochemical processes controlling the Venusian tropospheric chemical composition, surface rock mineral assemblages and the volatile element distribution in the atmosphere and planetary crust are discussed. In discussing the differentiation of volatiles in the formation of Venus and its atmosphere, it is noted that the isotopic ratios of the atmospheric gases indicate that the Venusian atmosphere cannot be regarded as the remnant of a protoplanetary nebula. The chemical history of inert volatiles differs drastically from that of chemically active volatiles.

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