Orbital Evolution and Migration of Giant Planets: Modeling Extrasolar Planets

@article{Trilling1998OrbitalEA,
  title={Orbital Evolution and Migration of Giant Planets: Modeling Extrasolar Planets},
  author={David E. Trilling and W. Benz and Tristan Guillot and Jonathan I. Lunine and William B. Hubbard and Adam S. Burrows},
  journal={The Astrophysical Journal},
  year={1998},
  volume={500},
  pages={428 - 439}
}
Giant planets in circumstellar disks can migrate inward from their initial (formation) positions. Radial migration is caused by inward torques between the planet and the disk, by outward torques between the planet and the spinning star, and by outward torques due to Roche lobe overflow and consequent mass loss from the planet. We present self-consistent numerical considerations of the problem of migrating giant planets. Summing torques on planets for various physical parameters, we find that… 

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