Model Evaporation of Chondrule Precursors in Nebular Shocks

Details Model Evaporation of Chondrule Precursors in Nebular Shocks Model Evaporation of Chondrule Precursors in Nebular Shocks

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpi....37.2249f&link_type=abstract

37th Annual Lunar and Planetary Science Conference, March 13-17, 2006, League City, Texas, abstract no.2249

Computer Science

3

Scientific paper

Evaporation rates from silicate liquids of model chondrule compositions
into a complementary solar gas rise with decreasing fo2 of formation of
the precursor. Minor evaporative losses of Fe, Mg and Si do not require
elevated ambient pressure or fO2.

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