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- W2141074409 abstract "C 60 has not yet been detected in primitive meteorites, a finding that could demonstrate its existence in the early solar nebular or as a component of presolar dust. However, other allotropes of carbon, diamond and graphite, have been isolated from numerous chondritic samples. Studies of the isotopic composition and trace element content and these forms of carbon suggest that they condensed in cireumstellar environments. Diamond may also have been produced in the early solar nebula and meteorite parent bodies by both low-temperature—low-pressure processes and shock events. Evidence for the occurrence of another carbon allotrope, with sp hybridized bonding, commonly known as carbyne, is presented." @default.
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- W2141074409 date "1993-04-15" @default.
- W2141074409 modified "2023-10-17" @default.
- W2141074409 title "Elemental carbon as interstellar dust" @default.
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- W2141074409 doi "https://doi.org/10.1098/rsta.1993.0042" @default.
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