2001Lunar and Planetary Science ConferenceRequires access

Presolar Grains in CM2 Chondrites

G. R. Huss, A. P. Meshik, C. M. Hohenberg

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Abstract

New abundance determinations for presolar diamond, SiC, and graphite in CM2 chondrites are presented and used to infer initial abundances in primitive solar-system material. Modifications of initial abundances reflect early-solar-system processes. Additional information is contained in the original extended abstract.

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What this paper is about

New abundance determinations for presolar diamond, SiC, and graphite in CM2 chondrites are presented and used to infer initial abundances in primitive solar-system material. Modifications of initial abundances reflect early-solar-system processes. Additional information is contained in the original extended abstract.

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Available abstract

New abundance determinations for presolar diamond, SiC, and graphite in CM2 chondrites are presented and used to infer initial abundances in primitive solar-system material. Modifications of initial abundances reflect early-solar-system processes. Additional information is contained in the original extended abstract.

Key concepts: Chondrite, Presolar grains, Astrobiology, Formation and evolution of the Solar System, Solar System, Meteorite, Abundance (ecology), Graphite

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