OUTWARD MIGRATION OF JUPITER AND SATURN IN EVOLVED GASEOUS DISKS

@article{DAngelo2012OUTWARDMO,
  title={OUTWARD MIGRATION OF JUPITER AND SATURN IN EVOLVED GASEOUS DISKS},
  author={G. D’Angelo and F. Marzari},
  journal={The Astrophysical Journal},
  year={2012},
  volume={757},
  pages={50}
}
  • G. D’Angelo, F. Marzari
  • Published 2012
  • Physics
  • The Astrophysical Journal
  • The outward migration of a pair of resonant-orbit planets, driven by tidal interactions with a gas-dominated disk, is studied in the context of evolved solar nebula models. The planets' masses, M{sub 1} and M{sub 2}, correspond to those of Jupiter and Saturn. Hydrodynamical calculations in two and three dimensions are used to quantify the migration rates and analyze the conditions under which the outward migration mechanism may operate. The planets are taken to be fully formed after 10{sup 6… CONTINUE READING
    50 Citations
    Planet formation in radiatively inefficient protoplanetary discs

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