Tidal synchronization of close-in satellites and exoplanets. II: Spin dynamics and extension to Mercury and exoplanet host stars
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Publication:748267
DOI10.1007/S10569-015-9624-5zbMath1322.70023arXiv1505.05384OpenAlexW3098119075MaRDI QIDQ748267
Publication date: 20 October 2015
Published in: Celestial Mechanics and Dynamical Astronomy (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1505.05384
Related Items (10)
Creep tide theory: equations for differentiated bodies with aligned layers ⋮ Fast numerics for the spin orbit equation with realistic tidal dissipation and constant eccentricity ⋮ Tides in a body librating about a spin-orbit resonance: generalisation of the Darwin-Kaula theory ⋮ Tidal effects in differentiated viscoelastic bodies: a numerical approach ⋮ A direct numerical verification of tidal locking mechanism using the discrete element method ⋮ Tidal synchronization of close-in satellites and exoplanets. III: Tidal dissipation revisited and application to Enceladus ⋮ Tidal synchronization of an anelastic multi-layered body: Titan's synchronous rotation ⋮ Tidal locking of habitable exoplanets ⋮ Rotation and figure evolution in the creep tide theory: a new approach and application to Mercury ⋮ Tidal synchronization of close-in satellites and exoplanets. II: Spin dynamics and extension to Mercury and exoplanet host stars
Cites Work
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- Tidal torques: a critical review of some techniques
- Tidal synchronization of close-in satellites and exoplanets. II: Spin dynamics and extension to Mercury and exoplanet host stars
- The flattenings of the layers of rotating planets and satellites deformed by a tidal potential
- Tidal friction in close-in satellites and exoplanets: the Darwin theory re-visited
- Large scale chaos and marginal stability in the solar system
- Asymptotic stability of synchronous orbits for a gravitating viscoelastic sphere
- Bodily tides near the 1:1 spin-orbit resonance: correction to Goldreich's dynamical model
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