Elemental and Isotopic Abundances of Carbon and Nitrogen in Meteorites

  • Monica M. Grady
  • Ian P. Wright
Part of the Space Sciences Series of ISSI book series (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.

Keywords

Isotopic Composition Parent Body Solar Nebula Carbonaceous Chondrite Iron Meteorite 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer Science+Business Media New York 2003

Authors and Affiliations

  • Monica M. Grady
    • 1
  • Ian P. Wright
    • 2
  1. 1.Dept. of MineralogyThe Natural History MuseumLondonUK
  2. 2.PSSRIThe Open UniversityWalton Hall, Milton KeynesUK

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