Condensation Origin of Some Metal Grains in CH Chondrites: Implications for the Formation of Metal in the CR-Clan

Details Condensation Origin of Some Metal Grains in CH Chondrites: Implications for the Formation of Metal in the CR-Clan Condensation Origin of Some Metal Grains in CH Chondrites: Implications for the Formation of Metal in the CR-Clan

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999lpi....30.1411m&link_type=abstract

30th Annual Lunar and Planetary Science Conference, March 15-29, 1999, Houston, TX, abstract no. 1411

Computer Science

Scientific paper

We report findings of large metal grains (~150 um) with distinct zoning
patterns in Ni, Co, Cr, and Si in CH chondrites which are consistent
with a condensation origin from a gas of solar composition.

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