Primary Reverse Oxygen-Isotope Evolution of Pyroxene in Compact Type A CAIs from the Efremovka and NWA-3118 CV3 Chondrites: Insights into Internal CAI Mixing Lines

Details Primary Reverse Oxygen-Isotope Evolution of Pyroxene in Compact Type A CAIs from the Efremovka and NWA-3118 CV3 Chondrites: Insights into Internal CAI Mixing Lines Primary Reverse Oxygen-Isotope Evolution of Pyroxene in Compact Type A CAIs from the Efremovka and NWA-3118 CV3 Chondrites: Insights into Internal CAI Mixing Lines

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.2415m&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.2415

Computer Science

Scientific paper

^1^6O-depleted Ti-Al-rich pyroxenes in compact Type A CAIs reflect the
composition of the perovsites from which they first formed. Perovsite
apparently exchanged oxygen very early, prior to melilite exchange and
to initial melting of the CAIs.

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