Possible in situ formation of meteoritic nanodiamonds in the early Solar System

Grains of dust that pre-date the Sun provide insights into their formation around other stars and into the early evolution of the Solar System. Nanodiamonds recovered from meteorites, which originate in asteroids, have been thought to be the most abundant type of presolar grain. If that is true, the...

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Veröffentlicht in:	Nature (London) 2002-07, Vol.418 (6894), p.157-159
Hauptverfasser:	DAI, Z. R, BRADLEY, J. P, JOSWIAK, D. J, BROWNLEE, D. E, HILL, H. G. M, GENGE, M. J
Format:	Artikel
Sprache:	eng
Schlagworte:	Accretion Asteroids Astronomy Cosmochemistry. Extraterrestrial geology Dust Earth sciences Earth, ocean, space Exact sciences and technology Meteorites. Tectites. Impactites Mineralogy Physics Solar system Stars
Online-Zugang:	Volltext
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