What the spectrum of radiation of stellar objects depends of?

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SUMMARY

The discussion centers on the development of a theory regarding the origins of fundamental forces, specifically focusing on the spectral radiation of stars and fogs in relation to their magnetic and gravitational fields. A table of spectra has been created to illustrate these relationships, but it requires quantification for comparison with existing databases. Participants are advised to study the luminosity-radius-temperature relationship and the Hertzsprung-Russell diagram to facilitate calculations of surface gravity and establish a gravity-spectrum relationship.

PREREQUISITES
  • Understanding of the Hertzsprung-Russell diagram
  • Knowledge of luminosity-radius-temperature relationships
  • Familiarity with magnetic field effects on stellar objects
  • Ability to quantify spectral data for comparison
NEXT STEPS
  • Research the Hertzsprung-Russell diagram in detail
  • Learn how to calculate surface gravity from stellar data
  • Investigate the impact of magnetic fields on stellar spectra
  • Quantify spectral data for comparative analysis with existing databases
USEFUL FOR

Astronomers, astrophysicists, and researchers interested in stellar radiation, fundamental forces, and the relationships between magnetic fields and spectral characteristics of celestial objects.

Michael F. Dmitriyev
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In the “ Theory development ” forum I develop my theory of a general origin of all fundamental forces. As an example of practical application of this theory I have developed the table of spectra of radiation of stars and fogs in dependence from a value of their magnetic and gravity fields. I ask to compare my results to an existing database and to make the conclusion about conformity.
The table is in the attachment.
Thanks.
 

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You will need to quantify the labels in your table, only then would it be possible to make a comparison.

Before you go collecting data on stars, I suggest that you read up about the luminosity-radius-temperature relationship, e.g.:
http://www-astronomy.mps.ohio-state.edu/~depoy/courses/AST162_LECTURE_NOTES/Unit1/hrdiag.html
and the Hertzsprung-Russell diagram, e.g.:
http://cassfos02.ucsd.edu/public/tutorial/HR.html

It will then be a simple exercise to calculate the surface gravity of any star in the H-R diagram; you will then have a gravity-spectrum relationship (the spectrum of a star is a much more detailed description than 'colour').

To begin with, you may assume all stars have 'weak' magnetic fields; once you've done the first stage of the research program I outlined here, you can start looking into variations due to magnetic field.

BTW, what do you mean by 'fogs'?
 
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