Measurement of Ti3+/Ti4+ Ratios in Pyroxene in Wark-Lovering Rims: Evidence for Formation in a Reducing Solar Nebula

Details Measurement of Ti3+/Ti4+ Ratios in Pyroxene in Wark-Lovering Rims: Evidence for Formation in a Reducing Solar Nebula Measurement of Ti3+/Ti4+ Ratios in Pyroxene in Wark-Lovering Rims: Evidence for Formation in a Reducing Solar Nebula

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpi....37.1772s&link_type=abstract

37th Annual Lunar and Planetary Science Conference, March 13-17, 2006, League City, Texas, abstract no.1772

Physics

Scientific paper

The pyroxene rim layers on CAIs are important recorders of nebular
conditions, including oxygen fugacity. Using XANES, we have directly
measured the Ti3+/Titot of pyroxene in the rim of an Allende fluffy Type
A inclusion.

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