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The Chelyabinsk meteorite sample of type LL5 was subjected to calcination in the specially constructed instrument in the temperature range 200–800°C in increments of 100°C. The composition of the obtained volatile constituents was examined on a chromatograph. Detected were: CO2, H2O, and N2 in concentrations of 5–40 μg/g of the sample; H2, CO, CH4, and H2S in concentrations of 0.1–2.0 μg/g. By observing changes in the selected component concentrations over time (up to 90 minutes), it was concluded that chemical reactions in the system between volatile components occur directly during outgassing.

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Solar System Research - The study of the degassing of primitive cosmic matter (in particular meteorites) allows us to better understand and evaluate the processes that occur during the formation of...  相似文献   
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Oceanology - Hydrocarbon gases (CH4, C2H4, C2H6, C3H6, C3H8, C4H8, n-C4H10, iC4H10, nC5H12, iC5H12, neo-C5H12), CO2, H2S, CH3SCH3, and COS were obtained from various marine sediment horizons at a...  相似文献   
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