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Formation and Evolution of Exoplanets

Protoplanetary Disk Physics → Numerical Simulation Methods

This advanced graduate-level path systematically covers the physical processes governing exoplanet formation and evolution, from protoplanetary disk physics to core accretion, disk migration, and dynamical interactions. It integrates planet formation theory with fluid dynamics and numerical simulation methods to explain observed exoplanet populations such as hot Jupiters and super-Earths.

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10 steps · 10 nodes · 3 stages

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Path Steps

10 steps · 3 stages. Click any step to inspect it and see it on the Path Map.

Stage 1

Foundation

4 steps

Stage 2

Core Concepts

3 steps

Stage 3

Advanced Topics

3 steps

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