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Analytical results for the material of the Chelyabinsk meteorite

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This paper presents the results of the mineralogical, petrographic, elemental, and isotopic analysis of the Chelyabinsk meteorite and their geochemical interpretation. It was shown that the meteorite can be assigned to LL5-group ordinary chondrites and underwent moderate shock metamorphism (stage S4). The Chelyabinsk meteorite contains a significant fraction (approximately one-third by volume) of shock-melted material similar in composition to the main volume of the meteorite. The results of isotopic analysis suggest that the history of meteorite formation included an impact event approximately 290 Ma ago.

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References

  1. J. T. Wasson and B. W. Kallemeyen, “Composition of chondrites,” Phil. Trans. R. Soc. Lond. A325, 535–544 (1988).

    Article  Google Scholar 

  2. E. Jarosewich, “Chemical analyses of meteorites: a compilation of stony and iron meteorite analyses,” Meteoritics 35, 323–337 (1990).

    Article  Google Scholar 

  3. S. B. Jacobsen and G. J. Wasserburg, “Sm-Nd isotopic evolution of chondrites,” Earth Planet. Sci. Lett. 50, 139–155 (1980).

    Article  Google Scholar 

  4. Yu. A. Kostitsyn, “Terrestrial and chondritic Sm-Nd and Lu-Hf isotopic systems: are they identical?” Petrology 12(5), 397–411 (2004).

    Google Scholar 

  5. A. E. Rubin, “Kamacite and olivine in ordinary chondrites: intergroup and intragroup relationships,” Geochim. Cosmochim. Acta 54, 1217–1232 (1990).

    Article  Google Scholar 

  6. F. Wlotzka, “Cr spinel and chromite as petrogenetic indicators in ordinary chondrites: equilibration temperatures of petrologic types 3.7 to 6,” Meteor. Planet. Sci. 40, 1673–1702 (2005).

    Article  Google Scholar 

  7. P. Kong and M. Ebihara, “The origin and nebular history of the metal phase of ordinary chondrites,” Geochim. Cosmochim. Acta 61, 2317–2329 (1997).

    Article  Google Scholar 

  8. D. Stoffler, K. Keil, and E. R. D. Scott, “Shock metamorphism in ordinary chondrites,” Geochim. Cosmochim. Acta 55, 3845–3867 (1991).

    Article  Google Scholar 

  9. K. Lodders and B. Fegley, The Planetary Scientific Companion (Oxford Univ. Press, New York, 1998).

    Google Scholar 

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Correspondence to E. M. Galimov.

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Original Russian Text © E.M. Galimov, V.P. Kolotov, M.A. Nazarov, Yu.A. Kostitsyn, I.V. Kubrakova, N.N. Kononkova, I.A. Roshchina, V.A. Alexeev, L.L. Kashkarov, D.D. Badyukov, V.S. Sevast’yanov, 2013, published in Geokhimiya, 2013, Vol. 51, No. 7, pp. 580–598.

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Galimov, E.M., Kolotov, V.P., Nazarov, M.A. et al. Analytical results for the material of the Chelyabinsk meteorite. Geochem. Int. 51, 522–539 (2013). https://doi.org/10.1134/S0016702913070100

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  • DOI: https://doi.org/10.1134/S0016702913070100

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