Cometary nuclei internal structure from early aggregation simulations

Abstract : A new model for the aggregation of cometesimals in the primordial solar nebula is proposed. Disruptive and sticking effects of impacts on the aggregates properties lead to particular inner geology, as well as layered surface of the resulting nuclei.
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Contributor : Catherine Cardon <>
Submitted on : Wednesday, August 15, 2012 - 12:29:34 PM
Last modification on : Wednesday, May 15, 2019 - 3:41:47 AM

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  • HAL Id : hal-00723884, version 1

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R. Botet, Jérémie Lasue, Anny Chantal Levasseur-Regourd, Edith Hadamcik. Cometary nuclei internal structure from early aggregation simulations. Asteroids, Comets, Meteors (ACM) 2012, proceedings, May 2012, Niigata, Japan. pp.6015. ⟨hal-00723884⟩

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