On the origin of Venus' atmosphere - Possible contributions from simple component mixtures and fractionated solar wind

Details On the origin of Venus' atmosphere - Possible contributions from simple component mixtures and fractionated solar wind On the origin of Venus' atmosphere - Possible contributions from simple component mixtures and fractionated solar wind

Apr 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988icar...74....3b&link_type=abstract

(Conference on the Origin and Evolution of Planetary and Satellite Atmospheres, Tucson, AZ, Mar. 10-14, 1987) Icarus (ISSN 0019-

Computer Science

2

Atmospheric Composition, Solar Planetary Interactions, Solar Wind, Venus Atmosphere, Abundance, Fractionation, Gas Mixtures, Rare Gases, Solar Activity Effects, Venus, Atmosphere, Formation, Origin, Mixing, Solar Wind, Fractionation, Carbon, Nitrogen, Rare Gases, Implantation, Adsorption, Abundance, Neon, Hypotheses, Models, Comparisons, Element Ratios, Argon, Concentration, Terrestrial Planets, Earth, Mars, Trapping, Temperature, Meteorites, Ci Chondrites

Scientific paper

Three-element correlation plots are used to assess the possible origin of C, N, and the noble gas elements in the atmosphere of Venus from various two-component mixtures and from elemental fractionation of solar gases during solar wind implantation and during low temperature adsorption. An origin of Venus' atmosphere by elemental fractionation of implanted solar wind gases into pre-Venus materials is approximately consistent with Ar, Kr, Xe, and N, but does not readily explain the higher abundance of C and the lower abundance of Ne. Some simple two-component mixtures seem consistent with most of the data, especially a mixture of an earth-like component with a lunar-like component that represents fractionated solar wind gases.

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