Calculate Total Energy Radiated by Sun During Evolution

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SUMMARY

The total energy radiated by the Sun during its evolution can be calculated by analyzing its internal energy changes and luminosity. Assuming the luminosity remains comparable to its present value, the energy radiated can be derived from the rate of change of internal energy. The discussion references specific calculations and methodologies outlined in the paper "The first million years of the Sun: A calculation of formation and early evolution of a solar-mass star" available at arXiv. Participants seek assistance in performing these calculations with provided numerical values.

PREREQUISITES
  • Understanding of stellar evolution concepts
  • Familiarity with luminosity and energy radiation principles
  • Basic knowledge of thermodynamics in astrophysics
  • Ability to interpret scientific papers, specifically in astrophysics
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  • Study the principles of stellar luminosity and its calculation
  • Learn about the thermodynamic processes in stellar evolution
  • Review the methodologies in the paper "The first million years of the Sun"
  • Explore energy conservation laws in astrophysical contexts
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Astronomers, astrophysics students, and researchers interested in stellar evolution and energy calculations related to solar and stellar models.

emilykay
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as the sun evolved it contracted, its internal energy changing fro x to y. what's the total energy radiated, assuming luminosity is comparable with present?


I understand that the rate of change of the internal energy = rate at which energy is radiated away by the star.. but i have been given exact numbers and i don't know what calculations to preform.

any help would be really good. thanks.
 
Astronomy news on Phys.org
Stars, like people, tend to be hot blooded in their youth:
http://arxiv.org/abs/astro-ph/0109051
The first million years of the Sun: A calculation of formation and early evolution of a solar-mass star
 

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