Calculate combined apparent magnitude of two stars

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SUMMARY

The combined apparent magnitude of a binary system consisting of two stars with apparent magnitudes of 3.0 and 4.0 can be calculated by converting these magnitudes to intensities and then adding the intensities together. The relevant equation is m-n=2.5 log(f(m)/f(n)), where f represents the flux or intensity of the stars. By using a reference magnitude of zero, one can compute the intensities of each star relative to a zero-magnitude star and then determine the combined magnitude by comparing the total intensity to that of the reference star.

PREREQUISITES
  • Understanding of apparent magnitude and its significance in astronomy
  • Familiarity with the concept of flux and intensity in relation to light
  • Knowledge of logarithmic functions and their application in calculations
  • Basic grasp of binary star systems and their properties
NEXT STEPS
  • Learn how to apply the formula for combined apparent magnitude in different scenarios
  • Study the relationship between flux and magnitude in more detail
  • Explore the concept of reference magnitudes in astronomical calculations
  • Investigate the effects of distance and brightness on apparent magnitude
USEFUL FOR

Astronomy students, astrophysics researchers, and anyone interested in understanding the calculations involved in determining the combined brightness of binary star systems.

Benzoate
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Homework Statement



What is the combined apparent magnitude o a binary system consisting of two stars of apparent magnitudes 3.0 and 4.0

Homework Equations



m-n=2.5 log(f(m)/f(n))

The Attempt at a Solution



I know m= 3 and n=4 ,or vice versa. I'm not sure what this problem means by combined magnitude. Do they mean I should add m and n together?
 
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Benzoate said:

Homework Statement



What is the combined apparent magnitude o a binary system consisting of two stars of apparent magnitudes 3.0 and 4.0

Homework Equations



m-n=2.5 log(f(m)/f(n))

The Attempt at a Solution



I know m= 3 and n=4 ,or vice versa. I'm not sure what this problem means by combined magnitude. Do they mean I should add m and n together?

Refer to your other post on the magnitude of a variable star for the discussion on the magnitude system.

What you want to do is convert your magnitudes to intensities, since the intensities of the two stars can be added to give the total intensity (or brightness or power) of the pair. This leaves the question of what to use for a basis. You can pick any reference magnitude, say, zero, and compute the intensity of each star relative to the intensity of a zero-magnitude star. You would then add the intensities of each star and now compare the total intensity to that of the zero-mag star to find the magnitude of the pair.
 
dynamicsolo said:
Refer to your other post on the magnitude of a variable star for the discussion on the magnitude system.

What you want to do is convert your magnitudes to intensities, since the intensities of the two stars can be added to give the total intensity (or brightness or power) of the pair. This leaves the question of what to use for a basis. You can pick any reference magnitude, say, zero, and compute the intensity of each star relative to the intensity of a zero-magnitude star. You would then add the intensities of each star and now compare the total intensity to that of the zero-mag star to find the magnitude of the pair.

Is the equation for intensity, f(n)/f(m)=100^(m-n)/5. for example , can I tlet my reference magnitude be 0 and magnitude of m(1) is 3 and for the second intensity, reference magnitude n is still zero and magnitude of m(2) is 4. Once i calculated the each of the intensities for the two stars , I proceed to add the two intensities of both stars?
 
Last edited:
Benzoate said:
Is the equation for intensity, f(n)/f(m)=100^(m-n)/5

I think your book or instructor is still using f from flux, but yes, that will work. (I just corrected a missing minus sign in my post in the other thread.)
 
Benzoate said:
can I tlet my reference magnitude be 0 and magnitude of m(1) is 3 and for the second intensity, reference magnitude n is still zero and magnitude of m(2) is 4. Once i calculated the each of the intensities for the two stars , I proceed to add the two intensities of both stars?

Somehow I got only the first line of this post when I went to reply to it... (?)

Yes, that is what I'm describing. You should get intensities which are between zero and 1, since they are the intensities relative to a brighter star...
 

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