Proton & Electron Speed in Stars: What You Need to Know

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SUMMARY

Protons and electrons within stars exhibit a wide range of velocities influenced by varying temperatures across different regions. The Maxwell–Boltzmann distribution serves as an effective model for approximating the speeds of these particles in stellar environments. While specific numerical values for particle speeds are not provided, understanding this distribution is crucial for analyzing particle dynamics in stars.

PREREQUISITES
  • Understanding of Maxwell–Boltzmann distribution
  • Basic knowledge of stellar structure and temperature gradients
  • Familiarity with particle physics concepts
  • Awareness of thermodynamic principles in astrophysics
NEXT STEPS
  • Research the application of Maxwell–Boltzmann distribution in astrophysics
  • Explore temperature profiles in different types of stars
  • Study the impact of particle velocities on stellar evolution
  • Investigate the relationship between temperature and pressure in stellar interiors
USEFUL FOR

Astronomers, astrophysicists, and students studying stellar dynamics and thermodynamics will benefit from this discussion.

PhDnotForMe
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How fast are protons and electrons moving within a star?
 
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They have a very wide range of velocities, with different velocity profiles for different regions of the star, since the star has regions of varying temperatures. Unfortunately I can't give you a number to go off of.
 
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