Tidal dissipation in stars and giant planets

Abstract

Astrophysical fluid bodies that orbit close to one another induce tidal distortions and flows that are subject to dissipative processes. The spin and orbital motions undergo a coupled evolution over astronomical timescales, which is relevant for many types of binary star, short-period extrasolar planetary systems and the satellites of the giant planets in the solar system. I review the principal mechanisms that have been discussed for tidal dissipation in stars and giant planets in both linear and nonlinear regimes. I also compare the expectations based on theoretical models with recent observational findings.

46 pages, 10 figures, to be published in Annual Review of Astronomy and Astrophysics, Volume 52

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• Observational imprints of tidal internal gravity wave dissipation in star-planet systems
• Modern tidal interaction models for rapid binary population synthesis: I. Methods
• The tidal interaction of an orbiting giant planet with a star near the Kraft break: the excitation of $r$-modes and the retention of orbital and spin angular momenta misalignment
• Characterizing the WASP-4 system with TESS and radial velocity data: Constraints on the cause of the hot Jupiter's changing orbit and evidence of an outer planet
• Breaking the Mass Inclination Degeneracy of Radial Velocity Measurements via Monitoring von Zeipel-Lidov-Kozai Cycles: Implications in the HD 41004 System
• Evolving Low- and Intermediate-Mass Binaries: Departures from Classical Theory
• Evolution of the ZTF SLRN-2020 star-planet merger
• Spin-spin coupling in stellar binaries
• How to measure tidal dissipation in long resonant chains