Computer Science
Scientific paper
Jun 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991gecoa..55.1709w&link_type=abstract
Geochimica et Cosmochimica Acta (ISSN 0016-7037), vol. 55, June 1991, p. 1709-1722. SNSF-supported research.
Computer Science
35
Allende Meteorite, Etching, Meteoritic Composition, Rare Gases, Argon Isotopes, Helium Isotopes, Krypton Isotopes, Neon Isotopes, Xenon Isotopes
Scientific paper
Results are presented from an analysis, in nearly pure form, of noble gases from the 'phase-Q' in an HF/HCl residue of the Allende C3V meteorite, using the closed-system stepped etching technique developed by Wieler et al. (1986) and Benkert et al. (1988) to extract noble gases from the residue. The results yield precise values of element and isotope abundances of all five noble gases in phase-Q, which is the major carrier of the planetary gases in carbonaceous chondrites. It was found that Ne-Q and Xe-Q in Allende are very similar to trapped gases in ureilites and in oxidizable carriers in several classes of ordinary chandrites, indicating that Q-gases are present in the formation locations of all these meteorites.
Anders Edward
Baur Heinrich
Lewis Roy S.
Signer Peter
Wieler Rainer
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