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Trace Element Composition and Classification of the Chinga Iron Meteorite

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Abstract

A complete microelement analysis of the Chinga meteorite was performed, and the possibility of attributing it together with a number of other iron meteorites into the IVC subgroup, which is transition between IVA and IVB is proposed.

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Authors and Affiliations

  1. Sobolev Institute of Geology and Mineralogy, Siberian Branch, Russian Academy of Sciences, Novosibirsk, 630090, Russia

    K. D. Litasov, I. S. Bazhan & N. P. Pokhilenko

  2. Novosibirsk State University, Novosibirsk, Russia

    D. S. Ponomarev

  3. University of Tokyo, Tokyo, Japan

    A. Ishikawa & T. Hirata

  4. Central Siberian Geological Museum, Novosibirsk, 630090, Russia

    N. M. Podgornykh

Authors
  1. K. D. Litasov
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  2. A. Ishikawa
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  3. I. S. Bazhan
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  4. D. S. Ponomarev
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  5. T. Hirata
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  6. N. M. Podgornykh
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  7. N. P. Pokhilenko
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Corresponding author

Correspondence to K. D. Litasov.

Additional information

Original Russian Text © K.D. Litasov, A. Ishikawa, I.S. Bazhan, D.S. Ponomarev, T. Hirata, N.M. Podgornykh, N.P. Pokhilenko, 2018, published in Doklady Akademii Nauk, 2018, Vol. 478, No. 1, pp. 81–85.

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Litasov, K.D., Ishikawa, A., Bazhan, I.S. et al. Trace Element Composition and Classification of the Chinga Iron Meteorite. Dokl. Earth Sc. 478, 62–66 (2018). https://doi.org/10.1134/S1028334X18010063

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  • DOI: https://doi.org/10.1134/S1028334X18010063

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