Tidal decay of close planetary orbits

F. A. Rasio*, C. A. Tout, S. H. Lubow, M. Livio

*Corresponding author for this work

Research output: Contribution to journalArticle

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Abstract

The 4.2 day orbit of the newly discovered planet around 51 Pegasi is formally unstable to tidal dissipation. However, the orbital decay time in this system is longer than the main-sequence lifetime of the central star. Given our best current understanding of tidal interactions, a planet of Jupiter's mass around a solar-like star could have dynamically survived in an orbit with a period as short as ∼10 hr. Since radial velocities increase with decreasing period, we would expect to find those planets close to the tidal limit first, and, unless this is a very unusual system, we would expect to find many more. We also consider the tidal stability of planets around more evolved stars, and we reexamine in particular the question of whether the Earth can dynamically survive the red giant phase in the evolution of the Sun.

Original languageEnglish (US)
Pages (from-to)1187-1191
Number of pages5
JournalAstrophysical Journal
Volume470
Issue number2 PART I
DOIs
StatePublished - Jan 1 1996

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Keywords

  • Celestial mechanics, stellar dynamics
  • Planetary systems
  • Solar system: General

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Rasio, F. A., Tout, C. A., Lubow, S. H., & Livio, M. (1996). Tidal decay of close planetary orbits. Astrophysical Journal, 470(2 PART I), 1187-1191. https://doi.org/10.1086/177941