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Does magnetic field modify tidal dynamics in the convective envelope of Solar mass stars?
Aurélie Astoul, Stéphane Mathis, Clément Baruteau +5
The energy dissipation of wave-like tidal flows in the convective envelope of low-mass stars is one of the key physical mechanisms that shape the orbital and rotational dynamics of…
Constraining the environment and habitability of TRAPPIST-1
Emeline Bolmont
The planetary system of TRAPPIST-1, discovered in 2016-2017, is a treasure-trove of information. Thanks to a combination of observational techniques, we have estimates of the radii…
Tidal heating in multilayer planets: Application to the TRAPPIST-1 system
Sylvain Breton, Emeline Bolmont, Gabriel Tobie +1
TRAPPIST-1 (Gillon et al. 2017) is an extremely compact planetary system: seven earth-sized planets orbit at distances lower than 0.07 AU around one of the smallest M-dwarf known i…
Planetary tidal interactions and the rotational evolution of low-mass stars. The Pleiades' anomaly
Florian Gallet, Emeline Bolmont, Jérôme Bouvier +2
The surface angular velocity evolution of low-mass stars is now globally understood and the main physical mechanisms involved in it are observationally quite constrained. Additiona…
Atmospheric reconnaissance of the habitable-zone Earth-sized planets orbiting TRAPPIST-1
J. de Wit, H. R. Wakeford, N. Lewis +14
Seven temperate Earth-sized exoplanets readily amenable for atmospheric studies transit the nearby ultracool dwarf star TRAPPIST-1 (refs 1,2). Their atmospheric regime is unknown a…
Early 2017 observations of TRAPPIST-1 with
Laetitia Delrez, Michael Gillon, Amaury H. M. J. Triaud +14
The recently detected TRAPPIST-1 planetary system, with its seven planets transiting a nearby ultracool dwarf star, offers the first opportunity to perform comparative exoplanetolo…