Properties, detectability and origin of interstellar diamonds in meteorites

Roy S. Lewis; Edward Anders; Bruce T. Draine

doi:10.1038/339117a0

Properties, detectability and origin of interstellar diamonds in meteorites

Roy S. Lewis
, Edward Anders
, Bruce T. Draine

Astrophysical Sciences

Research output: Contribution to journal › Article › peer-review

185 Scopus citations

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.

Original language	English (US)
Pages (from-to)	117-121
Number of pages	5
Journal	Nature
Volume	339
Issue number	6220
DOIs	https://doi.org/10.1038/339117a0
State	Published - 1989

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title = "Properties, detectability and origin of interstellar diamonds in meteorites",

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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journal = "Nature",

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T1 - Properties, detectability and origin of interstellar diamonds in meteorites

AU - Lewis, Roy S.

AU - Anders, Edward

AU - Draine, Bruce T.

PY - 1989

Y1 - 1989

N2 - 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.

AB - 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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U2 - 10.1038/339117a0

DO - 10.1038/339117a0

M3 - Article

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SN - 0028-0836

VL - 339

SP - 117

EP - 121

JO - Nature

JF - Nature

IS - 6220

ER -

Properties, detectability and origin of interstellar diamonds in meteorites

Abstract

All Science Journal Classification (ASJC) codes

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