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

Mario Trieloff (), Elmar K. Jessberger, Ingrid Herrwerth, Jens Hopp, Christine Fiéni, Marianne Ghélis, Michèle Bourot-Denise and Paul Pellas
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Mario Trieloff: Mineralogisches Institut der Universität Heidelberg
Elmar K. Jessberger: Institut für Planetologie, Westfälische Wilhelms-Universität
Ingrid Herrwerth: Max-Planck-Institut für Kernphysik
Jens Hopp: Mineralogisches Institut der Universität Heidelberg
Christine Fiéni: Laboratoire de Minéralogie du Muséum
Marianne Ghélis: Laboratoire de Minéralogie du Muséum
Michèle Bourot-Denise: Laboratoire de Minéralogie du Muséum
Paul Pellas: Laboratoire de Minéralogie du Muséum

Nature, 2003, vol. 422, issue 6931, 502-506

Abstract: Abstract 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

Date: 2003
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DOI: 10.1038/nature01499

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