Computer Science
Scientific paper
Jan 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998gecoa..62..301o&link_type=abstract
Geochimica et Cosmochimica Acta, vol. 62, p. 301
Computer Science
20
Rare Gases, Solar System Evolution, Meteoritic Composition, Geochemistry, Solar Wind, Gas Composition, Chemical Fractionation, Abundance, Energetic Particles, Solar Corpuscular Radiation, Xenon Isotopes, Neon Isotopes, Argon Isotopes, Krypton Isotopes
Scientific paper
The objective of this paper is to selectively review available data for noble gases for the Earth and meteorites (the Q component) and for the sun (solar wind) and to try to evaluate evolutionary scenarios which are not only compatible with terrestrial data but are also in harmony with the cosmochemical evolution of the solar system. The character of terrestrial noble gases does not at all emerge naturally from broader models of the origin of the solar system, but instead requires a variety of more or less arbitrary assumptions. In some cases hypotheses are suggested to account for noble gas observations which, if substantiated, would serve as strong constraints on models of the origin and early history of the solar system.
Marty Bernard
Ozima Minoru
Podosek Frank A.
Wieler Rainer
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