Tidal dissipation at arbitrary eccentricity and obliquity

Icarus

Volumn 193, Issue 2, 2008, Pages 637-640

  Wisdom, Jack ^a  

^a MASSACHUSETTS INSTITUTE OF TECHNOLOGY   (United States)

Author keywords

dynamics; Extrasolar planets; Satellites; solid body; Tides

Indexed keywords

EID: 38849110464     PISSN: 00191035     EISSN: 10902643     Source Type: Journal    
DOI: 10.1016/j.icarus.2007.09.002     Document Type: Article

References (9)

1. Garrick-Bethell I., Wisdom J., and Zuber M.T. Evidence for a past high eccentricity lunar orbit. Science 313 (2006) 652-655
2. Levrard B., Correia A.C.M., Chabrier G., Baraffe I., Selsis F., and Laskar J. Tidal dissipation within hot Jupiter: A new appraisal. Astron. Astrophys. 462 (2007) L5-L8
3. Mignard F. The evolution of the lunar orbit revisited, II. Moon Planets 23 (1980) 185-201
4. Peale S.J., and Cassen P. Contribution of tidal dissipation to lunar thermal history. Icarus 36 (1978) 245-269
5. Peale S.J., and Gold T. Rotation of the planet Mercury. Nature 206 (1965) 1240-1241
6. Peale S.J., Cassen P., and Reynolds R. Melting of Io by tidal dissipation. Science 203 (1979) 892-894
7. Plummer H.C. An Introductory Treatise on Dynamical Astronomy (1960), Dover, New York
8. Winn J.N., and Holman M.J. Obliquity tides on hot Jupiters. Astrophys. J. 628 (2005) L159-L162
9. Wisdom J. Spin-orbit secondary resonance dynamics of Enceladus. Astron. J. 128 (2004) 484-491