Redox History of Early Solar System Planetesimals Recorded in the D'Orbigny Angrite

Details Redox History of Early Solar System Planetesimals Recorded in the D'Orbigny Angrite Redox History of Early Solar System Planetesimals Recorded in the D'Orbigny Angrite

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.2436k&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.2436

Physics

Scientific paper

V-valence state oxybarometry of the D’Orbigny angrite show that
the crystalline and cavity pyroxenes in the rock formed at ~IW -
0.7, but that cross-cutting glass formed at IW + 2.9. Oxidation of the
glass may be due to lowered H_2 on the parent body.

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