Obliquity tides on hot Jupiters

Joshua N. Winn, Matthew J. Holman

Research output: Contribution to journalArticle

72 Scopus citations

Abstract

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.

Original languageEnglish (US)
Pages (from-to)L159-L162
JournalAstrophysical Journal
Volume628
Issue number2 II
DOIs
StatePublished - Aug 1 2005
Externally publishedYes

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Keywords

  • Celestial mechanics
  • Planetary systems: formation
  • Planets and satellites: formation
  • Stars: individual (HD 209458)

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