Formation of Oxygen Isotope Reservoirs by Mixing Chondritic Components

Details Formation of Oxygen Isotope Reservoirs by Mixing Chondritic Components Formation of Oxygen Isotope Reservoirs by Mixing Chondritic Components

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpi....37.1944h&link_type=abstract

37th Annual Lunar and Planetary Science Conference, March 13-17, 2006, League City, Texas, abstract no.1944

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D17O is controlled by the abundance of CAIs in CC and of type II
chondrules in OC, and D18O =d18O - d17O by the abundance of matrix in
all groups. Calculated D17O and D18O reproduce measured values.
Chondrite groups originated by mixing isotopically distinct petrologic
components.

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