Gas-Melt Interaction Experiments at High Temperature and High SiO(g) Partial Pressure — Implication of Melt Composition to Chondrule Formation

Details Gas-Melt Interaction Experiments at High Temperature and High SiO(g) Partial Pressure — Implication of Melt Composition to Chondrule Formation Gas-Melt Interaction Experiments at High Temperature and High SiO(g) Partial Pressure — Implication of Melt Composition to Chondrule Formation

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.1160k&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.1160

Physics

Scientific paper

We conducted new silica evaporation/condensation experiments to explore
solar nebular gas-melt interaction. Olivine starting matters resulted in
formation of pyroxene phases and Si-rich rims. Chondrule formation in
nebular regions with high P(SiO) is supported.

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