Condensation of the High-FeO Silicates in Primitive Chondrites: Still a Problem

Details Condensation of the High-FeO Silicates in Primitive Chondrites: Still a Problem Condensation of the High-FeO Silicates in Primitive Chondrites: Still a Problem

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.1448f&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.1448

Physics

2

Scientific paper

Olivine with significant XFa cannot form in water-rich solar gas, even
using new, higher Fe-Mg diffusion coefficients. It could form if
supersaturation of Fe metal occurred, but this is unlikely due to
homogeneous condensation of more refractory phases.

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