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Could star-planet magnetic interactions lead to planet migration and influence stellar rotation ?
Jérémy Ahuir, Antoine Strugarek, Allan-Sacha Brun +5
The distribution of hot Jupiters, for which star-planet interactions can be significant, questions the evolution of exosystems. We aim to follow the orbital evolution of a planet a…
Revised mass-radius relationships for water-rich rocky planets more irradiated than the runaway greenhouse limit
Martin Turbet, Emeline Bolmont, David Ehrenreich +5
Mass-radius relationships for water-rich rocky planets are usually calculated assuming most water is present in condensed (either liquid or solid) form. Planet density estimates ar…
Does magnetic field impact tidal dynamics inside the convective zone of low-mass stars along their evolution?
A. Astoul, S. Mathis, C. Baruteau +5
The dissipation of the kinetic energy of wave-like tidal flows within the convective envelope of low-mass stars is one of the key physical mechanisms that shapes the orbital and ro…
Final spin states of eccentric ocean planets
Pierre Auclair-Desrotour, Jérémy Leconte, Emeline Bolmont +1
Eccentricity tides generate a torque that can drive an ocean planet towards asynchronous rotation states of equilibrium when enhanced by resonances associated with the oceanic tida…
The runaway greenhouse radius inflation effect - An observational diagnostic to probe water on Earth-size planets and test the Habitable Zone concept
Martin Turbet, David Ehrenreich, Christophe Lovis +2
Planets similar to Earth - but slightly more irradiated - are expected to enter into a runaway greenhouse state, where all surface water rapidly evaporates, forming an optically th…
Correction to: Effect of the rotation and tidal dissipation history of stars on the evolution of close-in planets
Emeline Bolmont, Stéphane Mathis
This is an erratum for the publication Bolmont & Mathis 2016 (Celestial Mechanics and Dynamical Astronomy, 126, 275-296, https://doi.org/10.1007/s10569-016-9690-3). There was a sma…