QUE97416 and A-88882094, Two CO3 Breccias: Evidence from Petrologic Subtypes Determined from Amoeboid Olivine Inclusions

Details QUE97416 and A-88882094, Two CO3 Breccias: Evidence from Petrologic Subtypes Determined from Amoeboid Olivine Inclusions QUE97416 and A-88882094, Two CO3 Breccias: Evidence from Petrologic Subtypes Determined from Amoeboid Olivine Inclusions

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.2918c&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.2918

Physics

Scientific paper

AOIs in QUE 97416 and Asuka -882094 have differing ratios of Fe:Mg
olivine which seems to indicate a range of subtypes from 3.2 to 3.6.
This can be best explained if these meteorites are brecciated
representatives of the CO3 parent body asteroid.

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