Origin of Olivines in Type I Chondrules: Constraints from Oxygen and Magnesium Isotopic Compositions

Details Origin of Olivines in Type I Chondrules: Constraints from Oxygen and Magnesium Isotopic Compositions Origin of Olivines in Type I Chondrules: Constraints from Oxygen and Magnesium Isotopic Compositions

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpi....37.1335c&link_type=abstract

37th Annual Lunar and Planetary Science Conference, March 13-17, 2006, League City, Texas, abstract no.1335

Physics

1

Scientific paper

O and Mg isotopes in Vigarano type I chondrules containing olivine-rich
granoblasctic clasts are consistent with an origin by melting of a
mixture of relict olivines and CAI-like material with melt continuously
interacting with the nebular gas.

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