Chromium Stable Isotope Fractionation in the Early Solar Nebula

Details Chromium Stable Isotope Fractionation in the Early Solar Nebula Chromium Stable Isotope Fractionation in the Early Solar Nebula

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007lpi....38.1406m&link_type=abstract

38th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXVIII), held March 12-16, 2007 in League City, Texas

Computer Science

1

Scientific paper

We find Cr in carbonaceous chondrites is isotopically heavier in the
order CI, CM, CO, CV and CK. This trend suggests that volatility
controlled isotopic fractionation in the early solar nebula and/or
mixing between two isotopic distinct components.

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