Depths of segregation of HI-TiO2 picrite mare glasses

Details Depths of segregation of HI-TiO2 picrite mare glasses Depths of segregation of HI-TiO2 picrite mare glasses

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997lpi....28..559h&link_type=abstract

Conference Paper, 28th Annual Lunar and Planetary Science Conference, p. 559.

Physics

1

Separation, Glass, Titanium Oxides, Lunar Soil, Basalt, Magnesium Oxides, Silicon Dioxide

Scientific paper

It is argued that the moon's primitive mare melts were saturated with both olivine and low-Ca pyroxene at their source. Experimental data are presented that furnish the data needed to approximate a phase diagram that illuminates the petrogenesis of mare basalt. The MgO-SiO2-TiO2 ternary liquidus at high pressure is taken as a 'template' for the present discussion.

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