CORDIS Project
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This project aims to understand the evaporation processes of exoplanets and their atmospheres to gain insights into planet formation. By combining theoretical models, simulations, and observations, it seeks to uncover the mass-loss rates and evolutionary patterns of various exoplanets.
Modern astronomy has truly entered the exoplanet era.
Although our knowledge of what planet formation produces has grown immensely thanks to observational advances, our actual understanding of the physical processes that give rise to planets and planetary systems is limited.
We now know most stars are unlike our own Sun, in that they host planets which orbit around their star with periods of months or shorter, yet many have volatile rich atmospheres.
These planets must result from a dominant (if…
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