The Condensation Origin of Some Metal in CH Chondrites: A Thermodynamic Model

Details The Condensation Origin of Some Metal in CH Chondrites: A Thermodynamic Model The Condensation Origin of Some Metal in CH Chondrites: A Thermodynamic Model

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999lpi....30.1613p&link_type=abstract

30th Annual Lunar and Planetary Science Conference, March 15-29, 1999, Houston, TX, abstract no. 1613

Physics

3

Scientific paper

Thermodynamic modeling shows that zoned metal grains in the CH chondrite
PAT91546 are pristine nebular condensates formed in the solar nebula.
Isolation of condensing metal caused by grain growth resulted in
condensation of Ni-poor metal in the grain rim.

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