Formation of the Galilean Satellites: Conditions of Accretion

@article{Canup2002FormationOT,
  title={Formation of the Galilean Satellites: Conditions of Accretion},
  author={Robin M. Canup and William Rankin. Ward},
  journal={The Astronomical Journal},
  year={2002},
  volume={124},
  pages={3404 - 3423}
}
  • R. Canup, W. Ward
  • Published 1 December 2002
  • Physics, Geology
  • The Astronomical Journal
We examine formation conditions for the Galilean satellites in the context of models of late-stage giant planet accretion and satellite-disk interactions. We first reevaluate the current standard, in which the satellites form from a "minimum mass subnebula" disk, obtained by augmenting the mass of the current satellites to solar abundance and resulting in a disk mass containing about 2% of Jupiter's mass. Conditions in such a massive and gas-rich disk are difficult to reconcile with both the… 

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