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Star Formation and Early Stellar Evolution

Thermodynamics and Ideal Gas Law → Main Sequence Initiation

This learning path guides undergraduate astronomy students through the physical processes that lead from interstellar gas to a main-sequence star. It covers the interstellar medium, molecular clouds, gravitational collapse, protostar formation, and the early evolutionary phases culminating in the main sequence. Prerequisites in thermodynamics and gravitational physics are integrated to build a solid conceptual foundation.

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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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