The matrices of unequilibrated ordinary chondrites - Implications for the origin and history of chondrites

Mathematics – Logic

Scientific paper

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Chondrites, Matrix Materials, Meteoritic Composition, Meteoritic Microstructures, Mineralogy, Electron Microscopy, Evolution, Metamorphism (Geology), Space Exploration, Meteorites, Chondrites, Matrix, Origin, History, Catalogs, Data, Procedure, Microprobe Analysis, Textures, Mineralogy, Composition, Photomicrographs, Fayalite, Opacity, Comparisons, Optical Properties, Metamorphism, Recrystallization, Olivines, Chondrules, Thermal Effects, Shock, Formation, Classification

Scientific paper

The matrices of 16 unequilibrated chondrites were examined by optical microscopy, an electron microprobe, and a scanning electron microscope. The fine-grained, opaque, silicate matrix of type 3 unequilibrated chondrites was compositionally, mineralogically, and texturally different from the chondrules and their fragments; it may be the low temperature condensate proposed by Larimer and Anders (1967, 1970). Each meteorite has been metamorphosed by a combination of processes including thermal metamorphism and the passage of shock waves; the appearance of each chondrite results from the temperature and pressure conditions which formed it, and subsequent metamorphic alterations.

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