Accretion temperature of the Tieschitz, H3, chondritic meteorite

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Chemical Composition, Chondrites, Meteorites, Mineral Deposits, Planetary Evolution, Temperature Effects, Abundance, Crystallization, Czechoslovakia, Energy Spectra, Glass, Minerals, Phase Diagrams, Tieschitz Meteorite, Chondrules, Chondrites, Origin, Olivines, Pyroxenes, Composition, Petrology, Meteorites, Metamorphism, Volatiles, Silicates, Geochemistry, Electron Microscopy, Nepheline, Accretion, Fractional Crystallization, Pressure Gradients, Viscosity

Scientific paper

The Tieschitz, H3, chondritic meteorite apparently formed as part of a
parent-body by the accretion of both molten and solid materials with a
mean temperature of 800 + or - 100 C, followed by slow cooling to lower
temperatures. The data argue against the currently accepted model of
equilibration with a cooling gas of solar composition.

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