Formation of Chondrites by Reaction of Dusty Ices with Solar Nebula Gas

Details Formation of Chondrites by Reaction of Dusty Ices with Solar Nebula Gas Formation of Chondrites by Reaction of Dusty Ices with Solar Nebula Gas

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpi....39.1821p&link_type=abstract

39th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXIX), held March 10-14, 2008 in League City, Texas.

Computer Science

1

Scientific paper

Components of chondritic meteorites are in extreme disequilibrium. Some
of these features can be explained by reaction of dusty ices from the
outer solar system with hot nebular gas, in particular variations in
oxygen fugacity and oxygen isotopes.

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