Origin of Lunar Ultramafic Green Glasses: Constraints from Phase Equilibrium Studies

Details Origin of Lunar Ultramafic Green Glasses: Constraints from Phase Equilibrium Studies Origin of Lunar Ultramafic Green Glasses: Constraints from Phase Equilibrium Studies

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999lpi....30.1035e&link_type=abstract

30th Annual Lunar and Planetary Science Conference, March 15-29, 1999, Houston, TX, abstract no. 1035

Computer Science

1

Scientific paper

The compositional variability displayed in Apollo 14 and 11 green
glasses was produced by fractional crystallization of olivine and
orthopyroxene combined with assimilation of sunken high-Ti lunar magma
ocean cumulates at 440 km depth.

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