Trace element partitioning between ilmenite, armalcolite and anhydrous silicate melt: Implications for the formation of lunar high-Ti mare basalts

Author:

van Kan Parker Mirjam,Mason Paul R.D.,van Westrenen Wim

Funder

European Science Foundation

Nederlandse Organisatie voor Wetenschappelijk Onderzoek

Publisher

Elsevier BV

Subject

Geochemistry and Petrology

Reference75 articles.

1. Exotic armalcolite and the origin of Apollo 11 ilmenite basalts;Anderson;Geochimica et Cosmochimica Acta,1971

2. The source region and melting mineralogy of high-titanium and low-titanium lunar basalts deduced from Lu–Hf isotope data;Beard;Geochimica et Cosmochimica Acta,1998

3. Ilmenite solubility in Lunar basalts as a function of temperature and pressure: Implications for petrogenesis;Beck;Lunar and Planetary Science Conference,2004

4. Prediction of crystal-melt partition-coefficients from elastic-moduli;Blundy;Nature,1994

5. The influence of oxygen fugacity on tungsten and molybdenum partitioning between silicate melts and ilmenite;Candela;Economic Geology and the Bulletin of the Society of Economic Geologists,1990

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