CORDIS Project
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This project focuses on modeling the interior structure and evolution of ice giant planets, Uranus and Neptune. It uses molecular dynamics simulations to explore material properties and thermal boundaries, aiming to improve our understanding of these planets and their role in the Solar System.
The ice giant planets Uranus and Neptune are believed to play a crucial role in the formation process of our Solar System and are prototypical for hundreds of exoplanets, so-called mini-Neptunes, which are discovered at ever increasing speed thanks to planet-hunting missions like Kepler, TESS, and PLATO.
Modeling the interior structure, magnetic dynamo, and thermal evolution of Uranus and Neptune has proven very challenging relying only on the Voyager 2 flyby data from the 1980s and ground-based…
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