Other
Scientific paper
Jul 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982geokh......933l&link_type=abstract
Geokhimiia, July 1982, p. 933-945. In Russian.
Other
Abundance, Isotopes, Planetary Composition, Rare Gases, Solar System, Thermonuclear Reactions, Astronomical Models, Atom Concentration, Chemical Fractionation, Chondrites, Isotopic Enrichment, Lunar Composition, Meteoritic Composition, Solar Wind
Scientific paper
To explain the variations observed in the isotopic composition of inert gases in objects of the solar system, a model is proposed that combines two types of substances, the types differing in their thermonuclear origin. Each type contains inert gases that differ in their isotopic composition; the atomic distribution of the gases in each type (solar and planetary), however, is identical. Intermediate values of the isotopic composition of the inert gases (and of other elements) are explained as a superposition of the end members of the distribution. A significant fractionation effect is observed for one of these end members. It is shown that the model can explain in2reases in the relative amounts of heavy isotopes of xenon and other gases, the isotopic composition of solar gases, the origin of inert gases in the lunar regolith, and inclusions in chondrites having correlated nuclear and fractionation effects.
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