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NASA NTRS · 19890023516

Phase equilibrium constraints on the howardite-eucrite-diogenite association

Abstract

Model determinations of fractional crystallization and equilibrium partial melting in the 0-10-kbar range have been performed for a series of compositions relevant to diogenite and eucrite petrogenesis. Olivine is found to react with diogenite parent liquids along the plagioclase-absent olivine/low-Ca pyroxene liquidus boundary under conditions of both fractional and equilibrium crystallization up to about 2 kbar. Olivine also reacts with eucritic liquids saturated with plagioclase and low-Ca pyroxene to pressures in excess of 2 kbar. The ability of simple fractional crystallization at 2 kbar to account for mineralogical and chemical features of the diogenite-eucrite association is discussed.

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BibTeXRIS

Longhi, John, Pan, Vivian. 1988-01-01. Phase equilibrium constraints on the howardite-eucrite-diogenite association. https://ntrs.nasa.gov/citations/19890023516

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