Reassessing the Titanium Valence State in the Wark-Lovering Rim of a Leoville CAI: Further Evidence for an Oxidizing Nebular Environment for Wark-Lovering Rim Formation

Details Reassessing the Titanium Valence State in the Wark-Lovering Rim of a Leoville CAI: Further Evidence for an Oxidizing Nebular Environment for Wark-Lovering Rim Formation Reassessing the Titanium Valence State in the Wark-Lovering Rim of a Leoville CAI: Further Evidence for an Oxidizing Nebular Environment for Wark-Lovering Rim Formation

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpi....39.2372d&link_type=abstract

39th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXIX), held March 10-14, 2008 in League City, Texas.

Physics

Scientific paper

We analyzed Leoville 144A Wark-Lovering rim fassaite to investigate the
claim that low-Ti3+ values are the result of spinel contamination. We
prove spinel contamination does not occur in our data set, and verify
that WL rims formed in a more oxidizing environment than CAIs.

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