Two types of primary inert gases in meteorites and possible processes governing their capture

Details Two types of primary inert gases in meteorites and possible processes governing their capture Two types of primary inert gases in meteorites and possible processes governing their capture

Jan 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976geokh.......93l&link_type=abstract

Geokhimiia, Jan. 1976, p. 93-102. In Russian.

Computer Science

Abundance, Fractionation, Meteoritic Composition, Rare Gases, Argon Isotopes, Helium Isotopes, Silicates, Solar Wind, Xenon Isotopes

Scientific paper

Analysis of data on the isotopic composition of primary inert gases in meteorites confirms the existence of a two-component structure of these gases. The differences observed in the relative atomic abundance of the gases, in the isotopic composition, and release temperature are indicative of a different origin for both types of gases. The nonfractionated gases of type B are captured by matter through introduction of solar wind ions into crystal lattice. The fractionated gases of type A are absorbed by matter (high-temperature minerals) through thermal impregnation during the cooling of silicate dust in the protoplanetary nebula. The characteristic atomic structure of type A gases is developed before capture through diffusion of circumsolar plasma ions in the magnetic field of the sun.

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