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Elemental and Isotopic Abundances of Carbon and Nitrogen in Meteorites

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Solar System History from Isotopic Signatures of Volatile Elements

Part of the book series: Space Sciences Series of ISSI ((SSSI,volume 16))

Abstract

We have taken an inventory of the elemental and isotopic abundances of major carbon-and nitrogen-bearing components in different groups of meteorites. Primary phases, inherited from the solar nebula, are frequently isotopically heterogeneous, and surprisingly resistant to modification through parent body processing. Even melted and recrystallised meteorites retain primordial carbon and nitrogen isotopic signatures.

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Authors and Affiliations

  1. Dept. of Mineralogy, The Natural History Museum, Cromwell Road, London, SW7 5BD, UK

    Monica M. Grady

  2. PSSRI, The Open University, Walton Hall, Milton Keynes, MK7 6AA, UK

    Ian P. Wright

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  1. Monica M. Grady
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  2. Ian P. Wright
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Editor information

Editors and Affiliations

  1. International Space Science Institute, CH-3012, Bern, Switzerland

    R. Kallenbach  & J. Geiss  & 

  2. DESPA, Observatoire de Paris, F-92195, Meudon Cedex, France

    T. Encrenaz

  3. Max-Planck-Institut für Kernphysik, D-69029, Heidelberg, Germany

    K. Mauersberger

  4. University of Hawaii at Manoa, Honolulu, HI, 96822, USA

    T. C. Owen

  5. CNRS-Muséum, Muséum d’Histoire Naturelle, F-75005, Paris, France

    F. Robert

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Grady, M.M., Wright, I.P. (2003). Elemental and Isotopic Abundances of Carbon and Nitrogen in Meteorites. In: Kallenbach, R., Encrenaz, T., Geiss, J., Mauersberger, K., Owen, T.C., Robert, F. (eds) Solar System History from Isotopic Signatures of Volatile Elements. Space Sciences Series of ISSI, vol 16. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-0145-8_15

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  • DOI: https://doi.org/10.1007/978-94-010-0145-8_15

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