SIMBAD references

2005ApJ...628L.159W - Astrophys. J., 628, L159-L162 (2005/August-1)

Obliquity tides on hot Jupiters.

WINN J.N. and HOLMAN M.J.

Abstract (from CDS):

Obliquity tides are a potentially important source of heat for extrasolar planets on close-in orbits. Although tidal dissipation will usually reduce the obliquity to zero, a nonzero obliquity can persist if the planet is in a Cassini state, a resonance between spin precession and orbital precession. Obliquity tides might be the cause of the anomalously large size of the transiting planet HD 209458b.

Abstract Copyright:

Journal keyword(s): Celestial Mechanics - Stars: Planetary Systems: Formation - Planets and Satellites: Formation - Stars: Individual: Henry Draper Number: HD 209458

Simbad objects: 2

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