Xenon and neon from acid-resistant residues of Inman and Tieschitz

Details Xenon and neon from acid-resistant residues of Inman and Tieschitz Xenon and neon from acid-resistant residues of Inman and Tieschitz

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991gecoa..55.2921n&link_type=abstract

Geochimica et Cosmochimica Acta (ISSN 0016-7037), vol. 55, Oct. 1991, p. 2921-2936.

Computer Science

7

Carbonaceous Chondrites, Chemical Composition, Fine Structure, Neon Isotopes, Xenon Isotopes, Abundance, Galactic Cosmic Rays, Ion Production Rates, Residues, Silicon Carbides

Scientific paper

Results are reported on Xe and Ne isotopic compositions of highly oxidized acid-resistant demineralized residues from the unequilibrated ordinary chondrites Inman (L3.4) and Tieschitz (H/L3.6). Comparisons with previous results, and between Inman and Tieschitz, indicate that, even though the basic structure of Xe-HL is similar among the ordinary chondrites and among the carbonaceous chondrites, there are significant differences in the fine structure and the relationships between these components. For instance, Xe-S was readily observable in oxidized Inman residues but not in Tieshitz, while separation of Xe-L from Xe-H occurred in Tieschitz but not in Inman.

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