Compositions of Relict Olivines and Pyroxenes in Micrometeorites: In Comparison with Unequilibrated Chondrites

Details Compositions of Relict Olivines and Pyroxenes in Micrometeorites: In Comparison with Unequilibrated Chondrites Compositions of Relict Olivines and Pyroxenes in Micrometeorites: In Comparison with Unequilibrated Chondrites

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009lpi....40.1501i&link_type=abstract

40th Lunar and Planetary Science Conference, (Lunar and Planetary Science XL), held March 23-27, 2009 in The Woodlands, Texas, i

Physics

Scientific paper

Relict olivines and pyroxenes survived the atmospheric entry heating
among Antarctic micrometeorites tend to be similar to the CR2 and CO3.0
chondrites rather than the CM2 and Tagish Lake chondrites.

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