After the Main Sequence
Section 7 of 8
The Full Low-Mass Path
Part 6: Putting the Full Low-Mass Path Together
The combined HR-diagram evidence from clusters and field stars shows a path: main-sequence turnoff, subgiant branch, red giant branch, horizontal branch or red clump, AGB stars, planetary nebulae, white dwarf cooling sequence. These are the observable signposts of low-mass stellar evolution.
The physical chain is now complete:
- Core hydrogen is exhausted.
- The helium core contracts and heats by the virial theorem.
- Hydrogen shell burning ignites around the inert core.
- The envelope expands because shell luminosity and transport bottlenecks reorganize the outer star.
- Helium ignites when the core reaches .
- A helium flash occurs if the core is degenerate.
- Core helium burning creates carbon, and some carbon captures helium to form oxygen.
- The carbon-oxygen core contracts after helium is exhausted.
- Double-shell burning on the AGB drives instability and mass loss.
- The envelope is ejected as a planetary nebula.
- A white dwarf remains, supported by electron degeneracy pressure.
The overall timing is also part of the model:
| Phase | Typical duration for a Sun-like star | Dominant energy source |
|---|---|---|
| Main sequence | Core H burning | |
| RGB ascent | H shell burning | |
| Core He burning | Core He burning + H shell | |
| AGB | He shell + H shell | |
| Planetary nebula | Ionized ejecta around hot core | |
| White dwarf cooling | No fusion; cooling only |
These timescales reflect the basic rule , so long phases have large fuel reservoirs and modest luminosities, while short phases are either high-luminosity burning stages or brief transient transitions.
Low-mass stars do not end by catastrophic collapse, and the HR diagram does not show unrelated classes of stars scattered by chance. It shows a physically connected sequence of structural states that low-mass stars pass through after core hydrogen exhaustion.