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Chemical Abundances in Meteorites

  • Conference paper
Cosmic Chemistry

Part of the book series: Reviews in Modern Astronomy ((MOD.ASTRONOMY,volume 1))

Abstract

Some 4.6 billion years ago contraction and subsequent collapse of an interstellar cloud led to the formation of the solar system. The ratio of heavy elements to hydrogen, increasing continuously in interstellar material, due to the addition of freshly synthesized material from stars, was frozen in for the solar system at this point of time.

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Author information

Authors and Affiliations

  1. Max-Planck-Institut für Chemie, Saarstr. 23, D-6500, Mainz, Fed. Rep. of Germany

    H. Palme

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  1. H. Palme
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Editor information

Editors and Affiliations

  1. Landessternwarte, Königstuhl, D-6900, Heidelberg 1, Fed. Rep. of Germany

    Gerhard Klare

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© 1988 Springer-Verlag Berlin Heidelberg

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Palme, H. (1988). Chemical Abundances in Meteorites. In: Klare, G. (eds) Cosmic Chemistry. Reviews in Modern Astronomy, vol 1. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-74188-3_2

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  • DOI: https://doi.org/10.1007/978-3-642-74188-3_2

  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-642-74190-6

  • Online ISBN: 978-3-642-74188-3

  • eBook Packages: Springer Book Archive

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