Stellar Radius & Effective Temperature

Click For Summary
SUMMARY

The discussion centers on the relationship between stellar radius and effective temperature for Main Sequence stars, utilizing the equations L=4πR²σT⁴ and L∝M³.5. The user proposes a solution involving the solar version of the equations to derive R=RΘ(√(L/LΘ))(TeffΘ/Teff)². However, guidance is sought on whether to eliminate luminosity by incorporating mass, as indicated by the mention of density, which is crucial for a complete understanding of the relationship.

PREREQUISITES
  • Understanding of stellar luminosity and its equations
  • Familiarity with the concept of Main Sequence stars
  • Knowledge of effective temperature in astrophysics
  • Basic grasp of algebraic manipulation of equations
NEXT STEPS
  • Study the derivation of the mass-luminosity relationship for stars
  • Learn about the implications of mean density on stellar properties
  • Explore the concept of effective temperature in stellar astrophysics
  • Investigate the role of solar parameters in astrophysical equations
USEFUL FOR

Astronomy students, astrophysicists, and educators seeking to deepen their understanding of stellar properties and relationships in Main Sequence stars.

Physics Dad
Messages
54
Reaction score
1
I have a question for my Astro homework and I am a little unsure as to whether I am going in the right direction

Question
Using an expression that relates luminosity, size and temperature of a star, and assuming all Main Sequence stars have the same mean density, determine the relationship between stellar radius and effective temperature.

Relevant equations
L=4πR2σT4
L∝M3.5

Attempt at a solution
My thinking is to use the solar version of the above equation and this one, dividing one by the other to get rid of the 4π and σ and making...

R=RΘ(√(L/LΘ))(TeffΘ/Teff)2

However I don't know if I am supposed to just have R and T with no other variable.

Any guidance would be appreciated.
 
Last edited:
Physics news on Phys.org
Physics Dad said:
My thinking is to use the solar version of the above equation and this one, dividing one by the other
I don't think that is the right line. The information regarding density implies you are supposed to use some fact concerning mass to eliminate luminosity. Your second Relevant Equation looks useful in that regard.
 

Similar threads

  • · Replies 1 ·
Replies
1
Views
1K
Replies
0
Views
1K
  • · Replies 6 ·
Replies
6
Views
3K
Replies
15
Views
2K
  • · Replies 2 ·
Replies
2
Views
2K
Replies
2
Views
2K
  • · Replies 11 ·
Replies
11
Views
2K
  • · Replies 11 ·
Replies
11
Views
2K
  • · Replies 1 ·
Replies
1
Views
3K
  • · Replies 1 ·
Replies
1
Views
1K