On the origins of trapped helium, neon and argon isotopic variations in meteorites--II. Carbonaceous meteorites

Details On the origins of trapped helium, neon and argon isotopic variations in meteorites--II. Carbonaceous meteorites On the origins of trapped helium, neon and argon isotopic variations in meteorites--II. Carbonaceous meteorites

Mar 1972

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1972gecoa..36..377b&link_type=abstract

Geochimica et Cosmochimica Acta, vol. 36, Issue 3, pp.377-394

Computer Science

87

Scientific paper

Data are presented from stepwise heating experiments on five carbonaceous chondrites: Alais, Ivuna, Orgueil, Cold Bokkeveld and Nogoya. The data indicate the presence of two isotopically distinct major trapped components, components A and B. Two additional components, `C' and `E,' were isolated on the basis of neon isotopic structure. Components B and C, found in. gas-rich meteorites, are attributed to ion implantation by the present day solar wind and solar flares respectively. Component A is interpreted as a mixture of component E and component D (Paper I), where component D is identified with the primitive solar wind and component E is assigned an extra solar system origin.

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