Planetary System Formation and Evolution

We use Earth and Solar System input of geophysical fluid dynamics and thermal evolution of solid planets and the tectonic, glacial and volcanic features that shape their surfaces to model and study a wide range of possible planets and moons inside and outside our own Solar System.

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Atmospheric Spectral Signatures    Engaging With Life on Earth    Habitable Environments    Planetary Environments    Planetary System Formation and Evolution    Technological Development and Missions   
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