Origin of High-Ti Lunar Ultramafic Glasses: Experimental Evidence from Melting of Magma Ocean Cumulates and Depths of Positive Buoyancy for Melts of Varying TI Content

Details Origin of High-Ti Lunar Ultramafic Glasses: Experimental Evidence from Melting of Magma Ocean Cumulates and Depths of Positive Buoyancy for Melts of Varying TI Content Origin of High-Ti Lunar Ultramafic Glasses: Experimental Evidence from Melting of Magma Ocean Cumulates and Depths of Positive Buoyancy for Melts of Varying TI Content

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999lpi....30.1807v&link_type=abstract

30th Annual Lunar and Planetary Science Conference, March 15-29, 1999, Houston, TX, abstract no. 1807

Physics

Scientific paper

Experimental melts of high-Ti magma ocean cumulates do not resemble
high-Ti ultramafic glasses. Densities of lunar high-Ti melts constrain
depth of origin.

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