Stellar Evolution: Pathways & Perturbations

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SUMMARY

The discussion centers on stellar evolution pathways and their representation on the Hertzsprung-Russell (HR) diagram. It is established that stars of similar mass and chemical composition generally follow comparable evolutionary trajectories. However, small perturbations, such as star spots, have minimal impact on the overall evolution, while high-mass stars may exhibit more unpredictable pathways. The conversation emphasizes the importance of averaging over numerous stars to mitigate variations caused by unmodeled factors like rotation rate and magnetic fields.

PREREQUISITES
  • Understanding of the Hertzsprung-Russell (HR) diagram
  • Knowledge of stellar mass and chemical composition
  • Familiarity with astrophysical perturbations and their effects
  • Basic concepts of stellar evolution theory
NEXT STEPS
  • Research the impact of rotation rate on stellar evolution
  • Explore the role of magnetic fields in high-mass stars
  • Study the effects of companion stars on stellar pathways
  • Investigate advanced models of stellar evolution for high-mass stars
USEFUL FOR

Astronomers, astrophysicists, and students of stellar dynamics who are interested in the complexities of stellar evolution and the factors influencing star trajectories.

Simfish
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stellar evolution pathways...?

I find this especially interesting since the trajectories of stars on the HR diagram are more or less based on this assumption.

But obviously, small perturbations can lead to major changes in the long-run. But it seems that most of those changes involve only a small fraction of mass of the star (for example, star spots don't seem to change the star significantly). But perhaps trajectories are more unpredictable for extremely high mass stars?
 
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Simfish said:
Will two stars of the exact same mass and chemical composition undergo identical stellar evolution pathways...?

I find this especially interesting since the trajectories of stars on the HR diagram are more or less based on this assumption.

No. They are based on the assumption that stars of similar mass and composition will follow similar stellar evolution pathways, and moreover, that a averaging things out over lots and lots of stars will minimize variations due to unmodeled effects such as rotation rate, magnetic field, companion stars, etc.
 

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