« Paleo-climate » simulation of Hot Jupiters

By adapting the 3D general circulation model DYNAMICO developed at LSCE to the study of exoplanets, the ERC-ATMO team has shown that the unexplained radius inflation of Hot Jupiters is the result of the long timescale meridional circulations that heat up the deep atmosphere. Thanks to the increased performances of the code and by using low resolutions (similarly to paleo-climate studies for Earth climate), simulations on a timescale of 1000 years  (usual runs in the literature used a timescale of ~1 year) demonstrate that the deep circulations induced by the irradiation in the outer atmosphere are sufficient to confine the heat in the interior of the planet and keep it "puffy". The full article detailing these simulations, and our analysis of the results, is available online as part of Issue 632 (December 2019) of Astronomy and Astrophysics.

Averaged temperature profile of the simulation showing the heating of the deep atmosphere on a time scale of 1000 years.

Stream function of the simulation: clockwise circulations on the meridional plane are shown in red and anticlockwise circulations are shown in blue. Additionally the zonally and temporally averaged zonal wind is plotted in black (solid = eastward, dashed = westward).

Recruitment of a postdoctoral researcher

Solène BULTEAU has recently joined Maison de la Simulation as a postdoctoral researcher to develop new numerical methods for stratified magneto-hydrodynamic in a 3D convection code called Ark. This postdoc position of 3 years is funded by the European ERC ATMO project. It aims at studying exo-planet atmosphere using numerical simulation to prepare the future observation campaign of the space telescope James Webb. The work of Solène on atmospheric convection will be used for stars, brown dwarf and exo-planets.