A note on the systematics of noble gas abundance ratios in the solar system

Computer Science – Emerging Technologies

Scientific paper

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Abundance, Planetary Atmospheres, Rare Gases, Solar System, Concentration (Composition), Gas Analysis, Solar Wind, Planets, Rare Gases, Abundance, Isotopic Ratios, Hypotheses, Atmosphere, Patterns, Models, Fractionation, Analysis, Calculations, Distance, Venus, Earth, Mars, Carbonaceous Chondrites, Mercury (Planet), Jupiter, Meteorites, C Chondrites, Stony Meteorites, Ci Chondrites, Saturn

Scientific paper

It is demonstrated that there is a general regularity in all noble gas elemental patterns in the atmospheres of the planets. A number of models are proposed to explain this, and these models are examined and judged. In order to explain the observed elemental gas ratios, it is proposed that they may have resulted from selective loss of noble gas from the initial atmospheres of the terrestrial or other planets; that they may be due to solar wind irradiation of the planets and their small precursor bodies; or the noble gases were imported by carrier grains with their peculiar abundance ratio already fixed.

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