Communication Dans Un Congrès Année : 2005

Volatiles enrichments and composition of Jupiter

Résumé

We use the giant planets extended core-accretion model of Alibert et al. (2004, 2005) and the clathrate hydrate trapping theory to calculate the enrichments in O, C, N, S, Xe, Ar and Kr with respect to their solar abundances in Jupiter's atmosphere.

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Dates et versions

hal-00131754 , version 1 (19-02-2007)

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Y. Alibert, O. Mousis, W. Benz. Volatiles enrichments and composition of Jupiter. 36th Annual Lunar and Planetary Science Conference, Mar 2005, League City, Texas, United States. pp.1181. ⟨hal-00131754⟩

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