Some trace element constraints on lunar basalt genesis

Details Some trace element constraints on lunar basalt genesis Some trace element constraints on lunar basalt genesis

Apr 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976lpsc....7.1659d&link_type=abstract

In: Lunar Science Conference, 7th, Houston, Tex., March 15-19, 1976, Proceedings. Volume 2. (A77-34651 15-91) New York, Pergamon

Computer Science

3

Basalt, Lunar Composition, Lunar Evolution, Lunar Rocks, Trace Elements, Abundance, Apollo Flights, Barium, Breccia, Chemical Analysis, Igneous Rocks, Mass Ratios, Potassium, Volatility

Scientific paper

It is found that the origin of low-K high-Ti basalts involves the partial melting of an ilmenite-rich cumulate, with little or no ilmenite remaining in the residue. High-K high-Ti basalts may derived by low volume partial melting of either an ilmenite-rich cumulate or a lower Ti source region. Low-Ti basalts have been produced from source regions that preserved 'whole moon' ratios of incompatible elements. KREEP or its source region have previously undergone ilmenite fractionation and removal.

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