Condensation origin of some metal grains in CH chondrites: Implications for the formation of metal in the CR-clan

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.


Presented at:
30th Annual Lunar and Planetary Science Conference, Houston, TX, USA, March 15-29, 1999
Year:
1999
Laboratories:




 Record created 2012-07-02, last modified 2018-03-17

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