Math 2.0

Astronomy and astrophysics Definition

Henyey track

Builds on Hayashi trackStellar structureKelvin–Helmholtz mechanismEffective temperature

Definition

Fix a stellar mass MM and a chemical composition. Consider the pre-main-sequence evolutionary path of a star of mass MM in the plane of log⁡Teff\log T_{\mathrm{eff}} and log⁡L\log L. The Henyey track of mass MM is the part of this path during which:

  1. the star is in stellar structure equilibrium with a radiative core;
  2. the star contracts and is powered by the Kelvin–Helmholtz mechanism, before core hydrogen burning supplies its luminosity.

Here LL is the luminosity and TeffT_{\mathrm{eff}} the effective temperature.

Remarks

The track starts where the star leaves its Hayashi track and ends at the zero-age main sequence. For a radiative star of constant opacity, scaling arguments give a luminosity nearly independent of the radius, which is why LL changes little while TeffT_{\mathrm{eff}} rises. Example: a star of one solar mass leaves its Hayashi track when a radiative core appears. It then moves to the left along its Henyey track until it reaches the main sequence. Non-example: a star of 0.20.2 solar masses stays fully convective until it reaches the main sequence, so its path is a Hayashi track and has no Henyey part.

Reading path

To understand this page from the ground up, read these 5 pages in order. The foundations come first.

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Each page uses the pages above it. The colour of the bar on a box shows how strong the evidence is, and the box also gives it as text. The list has the same pages.
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  1. Effective temperature concept
  2. Hayashi track concept
  3. Kelvin–Helmholtz mechanism concept
  4. Stellar structure concept
  5. Henyey track definition

Further reading

  1. Web https://en.wikipedia.org/wiki/Henyey_track
About this page
TagX95A7HME0J
URIm2://X95A7HME0J
Kinddefinition
WritingW0 stub
MSC85A15
DefinesHenyey track
UsesHayashi track, Stellar structure, Kelvin–Helmholtz mechanism, Effective temperature
Changed3 November 2026

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