A comparative study of the isotopic composition of xenon in the new meteorite Kaydun and in the carbonaceous chondrites Mighei /C2M/, Kainsaz /C 30/ and Efremovka /C 3V/

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Carbonaceous Chondrites, Meteoritic Composition, Xenon Isotopes, Annealing, Chemical Fractionation, Degassing, Metamorphism (Geology), Rare Gases

Scientific paper

On the basis of preliminary data, the meteorite Kaydun, which fell to earth on December 30, 1980, can be classified as C2-C3. The degassing curve of the element has three maxima, which is typical of most carbonaceous chondrites. The isotopic composition is found to vary with annealing. The xenon in the meteorite comprises no fewer than three components: Xe-Z and Xe-P (products of mass fractionation) and Xe-X (which comprises spallogenic xenon and a product of the fission of Pu-244). The formation interval for the Kaydun chondrite is greater than that for the chondrites of C2M Mighei, C 30 Kainsaz, and C 3V Efremovka.

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