Petrology of the Yamato meteorites /j/, /k/, /l/, and /m/ from Antarctica

Mathematics – Logic

Scientific paper

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Achondrites, Chondrites, Meteoritic Composition, Petrology, Abundance, Antarctic Regions, Chemical Analysis, Microstructure, Mineralogy, Olivine, Pyroxenes, X Ray Fluorescence

Scientific paper

A petrological study of four meteorites is presented. The meteorites are a H-4 chondrite (Yamato 7301), a howardite (Yamato 7308), and two L-5 chondrites (Yamato 7304 and 7305). Meteorite pyroxenes and olivines are characterized. The howardite is a polymict breccia of diogenite and eucrite clasts, and the howardite pyroxenes form a definite trend probably related to fractional crystallization of the parental magma of the achondrite. High-temperature oligoclase is found in the chondrites while anorthite is found in the howardite. Intergrowth of nickel-iron, troilite, chromite, and rarely ilmenite is observed. Bulk composition and genetic implications are discussed.

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