Oxygen Isotope Micro-Distribution vs. Composition in Melilite/Fassaite in the Allende CAI 7R-19-1: A New Evidence for Multiple Heating

Details Oxygen Isotope Micro-Distribution vs. Composition in Melilite/Fassaite in the Allende CAI 7R-19-1: A New Evidence for Multiple Heating Oxygen Isotope Micro-Distribution vs. Composition in Melilite/Fassaite in the Allende CAI 7R-19-1: A New Evidence for Multiple Heating

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999lpi....30.1538i&link_type=abstract

30th Annual Lunar and Planetary Science Conference, March 15-29, 1999, Houston, TX, abstract no. 1538

Physics

1

Scientific paper

The heterogeneous distributions of O within a fassaite, and between
gehlenitic and akermanite-rich melilite in 7R-19-1, an Allende CAI
measured by micro-analysis with SIMS, showed evidence for multiple
heating in the primitive solar nebula.

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