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The Structure of the Solar Nebula From Cometary Composition

Published online by Cambridge University Press:  30 March 2016

D. Bockelée-Morvan
Affiliation:
Observatoire de Paris, 5 place Jules Janssen, F-92195, Meudon, France
F. Hersant
Affiliation:
Institut für Theoretische Astrophysik, Tiergartenstr. 15, D-69121, Heidelberg, Germany
D. Gautier
Affiliation:
Observatoire de Paris, France
J.-M. Huré
Affiliation:
Observatoire de Paris and Université de Paris 7, France

Abstract

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This paper presents an interpretation of cometary compositional data in the frame of an evolutionary 2D turbulent model of the Solar Nebula: D/H ratios, crystalline silicates and N2/CO deficiency.

Information

Type
I. Joint Discussions
Copyright
Copyright © Astronomical Society of Pacific 2005