Tidal friction in close-in satellites and exoplanets: the Darwin theory re-visited
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Publication:931235
DOI10.1007/s10569-008-9133-xzbMath1342.70038arXiv0712.1156OpenAlexW2083364693MaRDI QIDQ931235
Sylvio Ferraz-Mello, Adrián Rodríguez, Hauke Hussmann
Publication date: 25 June 2008
Published in: Celestial Mechanics and Dynamical Astronomy (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/0712.1156
ExoplanetsSatellitesCapture into 1:1 resonanceDarwin's theoryEnergy dissipationOrbit evolutionStationary rotationSynchronous rotationTidal friction
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Cites Work
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- Tidal torques: a critical review of some techniques
- The \(3:2\) spin-orbit resonant motion of Mercury
- The Effect of Tidal Friction on Eccentricity and Inclination
- The evolution of the lunar orbit revisited, II
- Some ideas on the freely decaying Navier-Stokes turbulence
- The evolution of the lunar orbit revisited. I
- On the Eccentricity of Satellite Orbits in the Solar System
- Methods of Celestial Mechanics
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