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3D modelling of the early Martian Climate under a denser CO2 atmosphere: Temperatures and CO2 ice clouds
Francois Forget, Robin Wordsworth, Ehouarn Millour +5
On the basis of geological evidence, it is often stated that the early martian climate was warm enough for liquid water to flow on the surface thanks to the greenhouse effect of a…
Effect of the stellar spin history on the tidal evolution of close-in planets
Emeline Bolmont, Sean N. Raymond, Jeremy Leconte +1
We investigate how the evolution of the stellar spin rate affects, and is affected by, planets in close orbits, via star-planet tidal interactions. To do this, we used a standard e…
A new vision on giant planet interiors: the impact of double diffusive convection
Jérémy Leconte, Gilles Chabrier
While conventional interior models for Jupiter and Saturn are based on the simplistic assumption of a solid core surrounded by a homogeneous gaseous envelope, we derive new models…