| # | Title | OpenStax Astronomy 2e Reading | Paired Lab/PS |
| 01 | The Equations of Stellar Structure: Mass, Momentum, and What Remains | Ch. 16.1–16.2 | Lab 01 / PS 01 |
| 02 | Equation of State and Opacity: What a Photon Fights Against | Not in OpenStax; derived from first principles |
| 03 | Radiative Energy Transport: How Heat Actually Gets Out | Ch. 16.2 (extends beyond OpenStax) | Lab 02 / PS 02 |
| 04 | Convection and the Schwarzschild Criterion | Ch. 16.2 (extends beyond OpenStax) |
| 05 | Nuclear Reactions I: The Proton-Proton Chain and the Gamow Peak | Ch. 16.3 | Lab 03 / PS 03 |
| 06 | Nuclear Reactions II: The CNO Cycle and Why Massive Stars Burn So Differently | Ch. 16.3 |
| 07 | The Mass-Luminosity Relation and Main-Sequence Lifetimes | Ch. 19.3 | Lab 04 / PS 04 |
| 08 | Stellar Models: Polytropes and Homology Relations | Not in OpenStax; derived from first principles |
| 09 | Post-Main-Sequence Evolution: Shell Burning and the Red Giant Branch | Ch. 21.1–21.2 | Lab 05 / PS 05 |
| 10 | Helium Burning: The Triple-Alpha Process and the Horizontal Branch | Ch. 21.3 |
| 11 | Late Stages of Low- and Intermediate-Mass Stars: AGB, Planetary Nebulae, and White Dwarf Formation | Ch. 21.4–21.5 | Lab 06 / PS 06 |
| 12 | Electron Degeneracy and the Chandrasekhar Mass | Ch. 22.1–22.2 |
| 13 | Massive Star Evolution and the Core-Collapse Supernova Mechanism | Ch. 22.3–22.5 | Lab 07 / PS 07 |
| 14 | Synthesis: Nucleosynthesis and Compact Remnants Across This Course | Ch. 22, Ch. 23 (read together) |