Electron microprobe study of a 'mysterite'-bearing inclusion from the Krymka LL-chrondrite

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Carbonaceous Chondrites, Electron Microscopy, Meteoritic Composition, Minerals, Granular Materials, Inclusions, Metal Oxides, Metal Particles, Olivine, Pyroxenes, Petrography, Abundance, Volatile Elements, C Chondrites, Mineralogy, Meteorites, Krymka Meteorite, Ll Chondrites, Inclusions, Composition, Electron Microprobe, Carbonaceous Chondrites, Olivines, Pyroxenes, Plagioclase, Classification, Metals, Element Ratios, Oxides, Grains, Chemistry, Mysterite, Formation, Condensation, Temperatures, Analysis, Tec

Scientific paper

The black inclusion from the Krymka LL3 chondrite previously found to contain 'mysterite' by Lewis et al. (1979) belongs to a hitherto unknown class of carbonaceous chondrites. Its olivine and pyroxene compositions, Fo 97-99 and En 96, respectively, are characteristic of carbonaceous chondrites and its plagioclase composition. An 100 is characteristic of C3's. It contains a peculiar group of Co-, Cr-rich metal grains whose compositions are similar, but not identical, to those in C2 chondrites. Its weight ratios of total Fe/SiO2 and SiO2/MgO are 0.74 and 1.43, respectively, and its atomic ratio of Si/Al is 10.7, exactly the same as in carbonaceous chondrites. Its bulk chemical composition is very close to that of the Murchison C2 chondrite. The association of mysterite with a special type of carbonaceous chondrite material suggests that mysterite formed by low-temperature condensation in a different region of the nebula from other carbonaceous chondrites.

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