Volatile inventories of the terrestrial planets

Physics – Geophysics

Scientific paper

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Planetology, Terrestrial Planets, Volatility, Comets, Erosion, Hydrodynamics, Mars (Planet), Meteorites, Planetary Atmospheres, Planets, Terrestrial Planets, Volatiles, Abundance, Concentration, Mars, Hydrodynamics, Escape, Atmosphere, Erosion, Origin, Source, Comets, Gases, Accretion, Snc Meteorites, Venus, Earth, Hydrogen, Rare Gases, Fractionation, Hypotheses, Review, Impacts, Ejection, Samples, Meteorite, Comparisons, Composition, Antarctic Meteorites, Eet Meteorites, Eeta79001

Scientific paper

Theoretical models and data analyses regarding the compositional and isotopic evolution of planetary volatile reservoirs are reviewed for the period 1983-1986. Both the loss of volatiles from the atmospheres (by hydrodynamic escape and/or atmospheric erosion) and the possible sources of these gases (comets and/or accretion from the primitve nebula) are considered, and evidence suggesting that the SNC meteorites may be of Martian origin is summarized in a table and discussed.

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