Tidal Dissipation in Rotating Giant Planets

@article{Ogilvie2004TidalDI,
  title={Tidal Dissipation in Rotating Giant Planets},
  author={Gordon I. Ogilvie and Douglas N. C. Lin},
  journal={The Astrophysical Journal},
  year={2004},
  volume={610},
  pages={477 - 509}
}
  • G. Ogilvie, D. Lin
  • Published 8 October 2003
  • Physics, Geology
  • The Astrophysical Journal
Many extrasolar planets orbit sufficiently close to their host stars that significant tidal interactions can be expected, resulting in an evolution of the spin and orbital properties of the planets. The accompanying dissipation of energy can also be an important source of heat, leading to the inflation of short-period planets and even mass loss through Roche lobe overflow. Tides may therefore play an important role in determining the observed distributions of mass, orbital period, and… 
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