36 citations · 54 across the 6 of their papers we have counts for
6 papers
The fate of Earth during the Sun's giant phases: New constraints from ab initio tidal modelling and AGB mass loss
M. Esseldeurs, S. Mathis, L. Decin
The long-term evolution of planetary systems around solar-type stars is governed by the interplay between stellar expansion, tidal interactions, and mass loss during the red giant…
Tidal Dissipation in Giant Planets
Jim Fuller, Tristan Guillot, Stephane Mathis +1
Tidal interactions between moons and planets can have major effects on the orbits, spins, and thermal evolution of the moons. In the Saturn system, tidal dissipation in the planet…
Solid tidal friction in multi-layer planets: Application to Earth, Venus, a Super Earth and the TRAPPIST-1 planets. Can a multi-layer planet be approximated as a homogeneous planet?
Emeline Bolmont, Sylvain N. Breton, Gabriel Tobie +3
With the discovery of TRAPPIST-1 and its seven planets within 0.06 au, the correct treatment of tidal interactions is becoming necessary. The eccentricity, rotation, and obliquity…
Layered semi-convection and tides in giant planet interiors - II. Tidal dissipation
Quentin André, Stéphane Mathis, Adrian J. Barker
Recent Juno observations have suggested that the heavy elements in Jupiter could be diluted throughout a large fraction of its gaseous envelope, providing a stabilising composition…
Layered semi-convection and tides in giant planet interiors
Q. André, S. Mathis, A. J. Barker
Layered semi-convection could operate in giant planets, potentially explaining the constraints on the heavy elements distribution in Jupiter deduced recently from Juno observations…
Layered semi-convection and tides in giant planet interiors - I. Propagation of internal waves
Quentin André, Adrian J. Barker, Stéphane Mathis
Layered semi-convection is a possible candidate to explain Saturn's luminosity excess and the abnormally large radius of some hot Jupiters. In giant planet interiors, it could lead…