Isotopic Records in Murray and Murchison Hibonites: Implications for the Oxygen Isotopic Reservoirs in the Early Solar System

Details Isotopic Records in Murray and Murchison Hibonites: Implications for the Oxygen Isotopic Reservoirs in the Early Solar System Isotopic Records in Murray and Murchison Hibonites: Implications for the Oxygen Isotopic Reservoirs in the Early Solar System

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001lpi....32.1576g&link_type=abstract

32nd Annual Lunar and Planetary Science Conference, March 12-16, 2001, Houston, Texas, abstract no.1576

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Oxygen isotope data for CM hibonites do not correlate with data for
other isotopes. The reservoir of the exotic Ti-50 got depleted during
the period of hibonite formation, which was not the case for exotic
O-16. Plausible scenarios are proposed.

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