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Consequences of semidiurnal thermal tides on hot Jupiters zonal mean flows
Pierre Auclair-Desrotour, Jérémy Leconte
Hot Jupiters are submitted to an intense stellar heating. The resulting thermal tides can torque their atmospheres into asynchronous rotation, while these planets are usually assum…
Tidal dissipation in deep oceanic shells: from telluric planets to icy satellites
Pierre Auclair-Desrotour, Stéphane Mathis, Jacques Laskar +1
Oceanic tides are a major source of tidal dissipation. They are a key actor for the orbital and rotational evolution of planetary systems, and contribute to the heating of icy sate…
Global climate modeling of Saturn's atmosphere. Part II: multi-annual high-resolution dynamical simulations
Aymeric Spiga, Sandrine Guerlet, Ehouarn Millour +9
The Cassini mission unveiled the intense and diverse activity in Saturn's atmosphere: banded jets, waves, vortices, equatorial oscillations. To set the path towards a better unders…
Differences in water vapor radiative transfer among 1D models can significantly affect the inner edge of the habitable zone
Jun Yang, Jeremy Leconte, Eric T. Wolf +8
An accurate estimate of the inner edge of the habitable zone is critical for determining which exoplanets are potentially habitable and for designing future telescopes to observe t…
Continuous reorientation of synchronous terrestrial planets controlled by mantle convection
Jérémy Leconte
A large fraction of known rocky exoplanets are expected to have been spun-down to a state of synchronous rotation, including temperate ones. Studies about the atmospheric and surfa…
The 0.8-4.5m broadband transmission spectra of TRAPPIST-1 planets
E. Ducrot, M. Sestovic, B. M. Morris +18
The TRAPPIST-1 planetary system represents an exceptional opportunity for the atmospheric characterization of temperate terrestrial exoplanets with the upcoming James Webb Space Te…