Noble gases in the Bells (C2) and Sharps (H3) chondrites

Details Noble gases in the Bells (C2) and Sharps (H3) chondrites Noble gases in the Bells (C2) and Sharps (H3) chondrites

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985metic..20..245z&link_type=abstract

Meteoritics (ISSN 0026-1114), vol. 20, pt. 1, June 30, 1985, p. 245-257.

Mathematics

Logic

4

Chondrites, Meteoritic Composition, Radioactive Age Determination, Rare Gases, Argon Isotopes, Cosmic Rays, Cosmochemistry, Mineralogy, Neon Isotopes, Radiogenic Materials, Meteorites, Rare Gases, Bells, Sharps, Cm2 Chondrites, H3 Chondrites, Mineralogy, Chemistry, Classification, Samples, Meteorite, Comparisons, Exposure Age, Parent Bodies, Radiogenic Elements, Cosmogenic Elements, Gases, Concentrations, Abundance, Metamorphism, Characteristics, Volatiles, Thermal Properties, History

Scientific paper

The Bells and Sharps chondrites are of uncertain classification in virtue of their mineralogical and chemical peculiarities, prompting the present elemental and isotopic measurements of the noble gases in them, together with such quantities derivable from them as cosmogenic exposure and gas retention ages, as well as primordial gas contents. The radiogenic and, above all, the cosmogenic gases link Bells to the C2 group, while Sharps is found to lie in the second largest peak of the H-chondrite distribution.

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