Tidal evolution and spin-orbit dynamics for bodies in the viscous regime
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Publication:6643691
DOI10.1007/S10569-024-10215-1MaRDI QIDQ6643691
Publication date: 26 November 2024
Published in: Celestial Mechanics and Dynamical Astronomy (Search for Journal in Brave)
Cites Work
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- Complete spin and orbital evolution of close-in bodies using a Maxwell viscoelastic rheology
- Dynamics of an isolated, viscoelastic, self-gravitating body
- Tidal synchronization of close-in satellites and exoplanets. II: Spin dynamics and extension to Mercury and exoplanet host stars
- The effects of deformation inertia (kinetic energy) in the orbital and spin evolution of close-in bodies
- Tidal evolution of the Keplerian elements
- Rotation and figure evolution in the creep tide theory: a new approach and application to Mercury
- Planetary tides: theories
- Librations of a body composed of a deformable mantle and a fluid core
- Tidal evolution for any rheological model using a vectorial approach expressed in Hansen coefficients
- The theory of figures of Clairaut with focus on the gravitational modulus: inequalities and an improvement in the Darwin-Radau equation
- Tidal synchronization of close-in satellites and exoplanets. III: Tidal dissipation revisited and application to Enceladus
- Viscoelastic tides: models for use in Celestial Mechanics
- The evolution of the lunar orbit revisited. I
- Explicit expansion of the three-body disturbing function for arbitrary eccentricities and inclinations
- Spin-orbit synchronization and singular perturbation theory
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