Modeling the Jovian subnebula: migration of proto-satellites

Details Modeling the Jovian subnebula: migration of proto-satellites Modeling the Jovian subnebula: migration of proto-satellites

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005sf2a.conf..205a&link_type=abstract

SF2A-2005: Semaine de l'Astrophysique Francaise, meeting held in Strasbourg, France, June 27 - July 1, 2005, Edited by F. Casoli

Astronomy and Astrophysics

Astrophysics

Scientific paper

We present an evolutionary turbulent model of the Jovian subnebula consistent with the extended core accretion formation models of Jupiter described by Alibert et al. (2005a). We calculate the thermodynamical conditions inside the subnebula, and the migration of proto-satellites. By tempting to reproduce the location vs. ice content of the Jovian satellites, we obtain constraints on the dissipation parameter inside the subnebula.

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