Correlation Between Texture and Oxygen Isotopic Systematics in CAIs from Acfer 094

Details Correlation Between Texture and Oxygen Isotopic Systematics in CAIs from Acfer 094 Correlation Between Texture and Oxygen Isotopic Systematics in CAIs from Acfer 094

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007lpi....38.1252f&link_type=abstract

38th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXVIII), held March 12-16, 2007 in League City, Texas

Physics

Scientific paper

Acfer 094 CAIs are generally 16O-rich. However, SIMS analysis and SCAPS
imaging of one CAI with a diopside rim indicate that the rim formed in a
16O-poor setting, implying stages of petrogenesis in distinct isotopic
environments in the solar nebula.

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