CORDIS Project
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The MagmaWorlds project investigates the evolutionary pathways of volatile-rich and volatile-poor super-Earth exoplanets using numerical simulations. It aims to understand how the internal structure and atmospheric conditions of these planets affect observable characteristics, enhancing our knowledge of their chemical…
The first low-mass exoplanet spectra from the James Webb Space Telescope (JWST) have toppled previous understanding on their internal structure and phase state, suggesting that mixing between the deep planetary interior and atmosphere affects key observables.
A newly emerging class of volatile-rich exoplanets, bridging the classes of super-Earths and sub-Neptunes, promises to enhance observational insights into atmosphere-interior feedbacks but requires novel models to interpret and predict obse…
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