Isotopic anomalies of Ne, Xe, and C in meteorites. I. Separation of carriers by density and chemical resistance.

Details Isotopic anomalies of Ne, Xe, and C in meteorites. I. Separation of carriers by density and chemical resistance. Isotopic anomalies of Ne, Xe, and C in meteorites. I. Separation of carriers by density and chemical resistance.

May 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988gecoa..52.1221t&link_type=abstract

Geochimica et Cosmochimica Acta, Vol. 52, No. 5, p. 1221 - 1234

Physics

10

Meteorites:Isotopic Abundances

Scientific paper

In an attempt to characterize the carriers of presolar noble gases, 19 - mainly non-colloidal - separates from the Murray and Murchison C2 chondrites were isotopically analyzed for Ne, Xe, and in several cases for C and N. Although most samples were stronlgy depleted in Xe-HL and enriched in Ne-E(H), Ne-E(L), and Xe-S, the separation methods failed to isolate the noble-gas carriers in pure form. Nonetheless, several new properties of the carriers were established.

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