Structure and thermal history of the H-chondrite parent asteroid revealed by thermochronometry

Our Solar System formed ∼4.6 billion years ago from the collapse of a dense core inside an interstellar molecular cloud. The subsequent formation of solid bodies took place rapidly. The period of

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Bibliographische Detailangaben
Veröffentlicht in:	Nature (London) 2003-04, Vol.422 (6931), p.502-506
Hauptverfasser:	Trieloff, Mario, Jessberger, Elmar K, Herrwerth, Ingrid, Hopp, Jens, Fiéni, Christine, Ghélis, Marianne, Bourot-Denise, Michèle, Pellas, Paul
Format:	Artikel
Sprache:	eng
Schlagworte:	Accretion Asteroids Cosmochemistry. Extraterrestrial geology Earth sciences Earth, ocean, space Exact sciences and technology Extraterrestrial geology Geochronology Isotope geochemistry. Geochronology Metamorphism Meteors & meteorites Rocks Thermodynamics
Online-Zugang:	Volltext
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Beschreibung
Zusammenfassung:	Our Solar System formed ∼4.6 billion years ago from the collapse of a dense core inside an interstellar molecular cloud. The subsequent formation of solid bodies took place rapidly. The period of
ISSN:	0028-0836 1476-4687
DOI:	10.1038/nature01499