Oxygen-Isotopic Compositions of Forsterite in an Accretionary Rim Around Ca, Al-rich Inclusion and in an Amoeboid Olivine Aggregate from the Reduced CV Chondrite Efremovka and Their Significance

Details Oxygen-Isotopic Compositions of Forsterite in an Accretionary Rim Around Ca, Al-rich Inclusion and in an Amoeboid Olivine Aggregate from the Reduced CV Chondrite Efremovka and Their Significance Oxygen-Isotopic Compositions of Forsterite in an Accretionary Rim Around Ca, Al-rich Inclusion and in an Amoeboid Olivine Aggregate from the Reduced CV Chondrite Efremovka and Their Significance

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001lpi....32.2016k&link_type=abstract

32nd Annual Lunar and Planetary Science Conference, March 12-16, 2001, Houston, Texas, abstract no.2016

Computer Science

5

Scientific paper

^16O-rich nebular gas is inferred from O-isotopic composition of
forsterites in an accretionary rim around compact Type A CAI and in an
amoeboid olivine aggregate from the reduced CV chondrite Efremovka.
Isotope exchange of melilite is also discussed.

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