Learning Path

Physics of Protoplanetary Disks

Fluid Dynamics Basics → Disk Evolution and Dispersal

14 Knowledge Nodes · 14 Learning Steps · v0 Active

A graduate-level learning path covering the fundamental physics governing protoplanetary disks: structure, accretion, magnetohydrodynamics, dust evolution, chemistry, and planet-disk interactions. Designed for exoplanet science students, it builds from fluid dynamics and MHD to advanced disk processes and observational connections.

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14 nodes19 edges1 relationships

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Path Nodes

14 learning steps · 3 phases. Click any step to inspect it and see it on the Path Map.

Phase 1

Foundation

5 steps

Phase 2

Core Concepts

5 steps

Phase 3

Advanced Topics

4 steps