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Properties, detectability and origin of interstellar diamonds in meteorites

Nature volume 339, pages 117–121 (1989)Cite this article

Abstract

Laboratory studies suggest that microdiamonds will be quite elusive in interstellar space, being detectable only if >10% of the carbon is present as diamond. The diamonds apparently formed by condensation in cool stellar atmospheres, and were then impregnated with isotopically anomalous noble gases, such as Xe, from a supernova.

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Authors and Affiliations

  1. Enrico Fermi Institute and Department of Chemistry, University of Chicago, Chicago, Illinois, 60637-1433, USA

    Roy S. Lewis & Edward Anders

  2. Princeton University Observatory, Princeton, New Jersey, 08544-1001, USA

    Bruce T. Draine

Authors
  1. Roy S. Lewis
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  2. Edward Anders
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  3. Bruce T. Draine
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Lewis, R., Anders, E. & Draine, B. Properties, detectability and origin of interstellar diamonds in meteorites. Nature 339, 117–121 (1989). https://doi.org/10.1038/339117a0

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