Native Silicon and Fe-Silicides from the Apollo 16 Lunar Regolith: Extreme Reduction, Metal-Silicate Immiscibility, and Shock Melting

Details Native Silicon and Fe-Silicides from the Apollo 16 Lunar Regolith: Extreme Reduction, Metal-Silicate Immiscibility, and Shock Melting Native Silicon and Fe-Silicides from the Apollo 16 Lunar Regolith: Extreme Reduction, Metal-Silicate Immiscibility, and Shock Melting

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.2231s&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.2231

Computer Science

1

Scientific paper

Native silicon and Fe-silicides occur in a complex anorthositic grain
from the Apollo 16 lunar regolith. We suggest formation of native
silicon and Fe-silicides result from metal-silicate immiscibility, most
likely the result of shock melting.

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