Petrogenesis of eucrite, howardite and diogenite meteorites

Details Petrogenesis of eucrite, howardite and diogenite meteorites Petrogenesis of eucrite, howardite and diogenite meteorites

Nov 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975natur.258..220s&link_type=abstract

Nature, vol. 258, Nov. 20, 1975, p. 220-222.

Astronomy and Astrophysics

Astronomy

11

Astronomical Models, Meteoritic Composition, Petrology, Stony Meteorites, Crystallization, Liquidus, Oxygen, Pressure Effects, Thermodynamic Properties

Scientific paper

Experimentally determined phase equilibria are related to the igneous processes which produced the eucrites and their associates. Melting experiments involving a sample of the Juvinas eucrite had been conducted at 1 atm total pressure and various oxygen fugacities. A projection of a low pressure liquidus diagram relevant to eucrite crystallization is presented. The possibility is considered that the eucrites may have formed by partial melting of the primitive material of the eucrite parent body.

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