How many M type stars equal the luminosity of one O type star?

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Discussion Overview

The discussion revolves around determining how many M-type stars would be needed to match the luminosity of a single O-type star, specifically focusing on the mass-luminosity relationship and the factors influencing stellar brightness.

Discussion Character

  • Technical explanation
  • Mathematical reasoning

Main Points Raised

  • One participant inquires about the equation needed to calculate the number of 0.75 Msolar main sequence stars required to equal the luminosity of a 3 Msolar O-type star.
  • Another participant suggests that the mass-luminosity relation can be used, stating that luminosity is proportional to mass raised to the power of 3.5.
  • A later reply notes that the mass-luminosity relation assumes similar composition among the stars, indicating that variations in helium and metal content can affect luminosity.

Areas of Agreement / Disagreement

Participants have not reached a consensus on the exact number of M-type stars needed, and multiple approaches to the problem are presented without resolution.

Contextual Notes

The discussion does not clarify the specific assumptions regarding stellar composition or the exact values needed for calculations, leaving some uncertainty in the application of the mass-luminosity relation.

blumfeld0
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Hello. what equation do i use to figure out how many .75*Msolar main sequence stars would it take to equal the luminosity of one 3*Msolar O tpe star?
I know O type are much brighter but how many times brighter?

thank you
 
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blumfeld0 said:
Hello. what equation do i use to figure out how many .75*Msolar main sequence stars would it take to equal the luminosity of one 3*Msolar O tpe star?
I know O type are much brighter but how many times brighter?

thank you
You ought to be able to get most of this info from links starting on http://www.astronomynotes.com/starprop/chindex.htm" .

or http://www.astro.caltech.edu/~kbundy/ay1page/lectures/class7.pdf".
 
Last edited by a moderator:
blumfeld0 said:
Hello. what equation do i use to figure out how many .75*Msolar main sequence stars would it take to equal the luminosity of one 3*Msolar O tpe star?
I know O type are much brighter but how many times brighter?

I would use a table, but if you can't find one, the mass-luminosity relation should be fine:

[tex]\frac{L}{L_{sun}} \propto (\frac{M}{M_{sun}})^{3.5}[/tex]
 
SpaceTiger said:
I would use a table, but if you can't find one, the mass-luminosity relation should be fine:

[tex]\frac{L}{L_{sun}} \propto (\frac{M}{M_{sun}})^{3.5}[/tex]


As a side note this requires that composition (hydrogen, helium, metal mass fractions) be the same. Higher helium content will mean higher luminosity as will lower metal content.
 

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