Chromium Isotopes in Chondrites and the Heterogeneous Accretion of the Solar Nebula

Details Chromium Isotopes in Chondrites and the Heterogeneous Accretion of the Solar Nebula Chromium Isotopes in Chondrites and the Heterogeneous Accretion of the Solar Nebula

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.2703d&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.2703

Physics

3

Scientific paper

There are different ɛ54Cr values in CC, EC and OC; the 54Cr
anomaly is a nuclear effect. Cr isotopes were not homogenized in the
nebula or in the parental molecular cloud. CAIs cannot form by
evaporation of chondritic materials.

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