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 …

We study tidal dissipation in stars with masses in the range 0.1–1.6 M⊙ throughout their
evolution, including turbulent effective viscosity acting on equilibrium tides and inertial …

Tidal interactions between moons and planets can have major effects on the orbits, spins,
and thermal evolution of the moons. In the Saturn system, tidal dissipation in the planet …

Io is the volcanically most active body in the Solar System and has a large surface heat flux,,.
The geological activity is thought to be the result of tides raised by Jupiter, but it is not known …

The inner moons of Jupiter and Saturn migrate outwards due to tidal energy dissipation
within the planets, the details of which remain poorly understood. We demonstrate that …

When main-sequence stars expand into red giants, they are expected to engulf close-in
planets,,,–. Until now, the absence of planets with short orbital periods around post …

We calculate the excitation and dissipation of low-frequency tidal oscillations in uniformly
rotating solar-type stars. For tidal frequencies smaller than twice the spin frequency, inertial …

The search for planets around white dwarf stars, and evidence for dynamical instability
around them in the form of atmospheric pollution and circumstellar disks, raises questions …

Tidal interactions between Saturn and its satellites play a crucial role in both the orbital
migration of the satellites and the heating of their interiors. Therefore, constraining the tidal …

The Sun's complex dynamics is controlled by buoyancy and rotation in the convection zone.
Large-scale flows are dominated by vortical motions and appear to be weaker than …