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WASp-121b at different phases as would be seen by an observer, modelled with the 3D SPARC/MITgcm.

The hot Jupiter WASP-121b at different phases as would be seen by an observer, modelled with the 3D SPARC/MITgcm.

Credit: Vivien Parmentier

Vivien Parmentier

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Research theme

  • Astronomy and astrophysics
  • Exoplanets and planetary physics

Sub department

  • Atmospheric, Oceanic and Planetary Physics

Research groups

  • Exoplanet atmospheres
  • Exoplanets and Stellar Physics
vivien.parmentier@physics.ox.ac.uk
Telephone: 01865282458
Atmospheric Physics Clarendon Laboratory, room 116
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