Astronomy and astrophysics Definition
Hayashi track
Builds on Stellar structureSchwarzschild criterion for convectionEffective temperature
Definition
Fix a stellar mass and a chemical composition. Consider the stellar structure models of mass that are convective from the centre to the photosphere. Here convective is meant in the sense of the Schwarzschild criterion, and the interior gradient is taken adiabatic. Let be the luminosity and the effective temperature. The Hayashi track of mass is the curve traced by these models, as their radius varies, in the plane of and .
Remarks
Matching an adiabatic interior to a photosphere whose opacity is dominated by negative hydrogen ions makes depend only weakly on , so the track is nearly vertical. Example: a newly formed star of one solar mass contracts down its Hayashi track, with around , until a radiative core appears. Non-example: the Sun today is not on its Hayashi track, since its core is radiative; only its outer envelope is convective. Models to the right of the track, at lower , would need a temperature gradient steeper than adiabatic, which convection removes at once, so such equilibria do not exist.
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Further reading
About this page
| Tag | FNY22W16F8 |
|---|---|
| URI | m2://FNY22W16F8 |
| Kind | definition |
| Writing | W0 stub |
| MSC | 85A15 |
| Defines | Hayashi track |
| Uses | Stellar structure, Schwarzschild criterion for convection, Effective temperature |
| Changed | 3 November 2026 |
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