Learning Path

Gravitational Microlensing in Exoplanet Science

Exoplanet Detection Methods I → Mass Determination from Microlensing

10 Knowledge Nodes · 10 Learning Steps · v0 Active

This path guides undergraduate astronomy students through the principles and applications of gravitational microlensing for detecting exoplanets. It covers the necessary physics background, the characteristics of microlensing light curves, how planets reveal themselves, and the methods used to analyze real events.

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Path Nodes

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

Phase 1

Foundation

4 steps

Phase 2

Core Concepts

3 steps

Phase 3

Advanced Topics

3 steps