Computer Science
Scientific paper
Aug 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982geokh.....1072l&link_type=abstract
Geokhimiia, Aug. 1982, p. 1072-1077. In Russian.
Computer Science
Chemical Composition, Isotopes, Rare Gases, Sun, Argon Isotopes, Plutonium 244, Solar Wind, Xenon Isotopes
Scientific paper
On the basis of data about the isotopic composition of inert gases in various objects of the solar system it is shown that the isotopic composition of solar xenon corresponds neither to the average isotopic composition of xenon in carbonaceous chondrites nor to the isotopic composition of lunar xenon type I extracted from the regolith. The isotopic composition of solar xenon is close to that of the earth's atmosphere and to lunar xenon type II. A significant portion of xenon in the regolith is not due to the solar wind irradiation. A lower initial ratio of Xe-136/Xe-130 (up to 1.5-1.6) leads to an increase in the concentration of Pu-244 in matter of the early solar system. The solar argon ratio of Ar-36/Ar-38 is probably greater than that of the earth's atmosphere.
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