Determining the individual magnitudes of two stars

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To determine the individual magnitudes of stars S1 and S2, first understand the apparent flux ratio, which indicates that S1 is twice as bright as S2. Given that the combined apparent brightness is 0.0 mag, you can express the brightness of S1 and S2 in terms of their fluxes. The relationship between brightness and magnitude is logarithmic, so you can convert the flux ratios into magnitude differences using the formula for magnitude difference based on brightness ratios. Additionally, consider how brightness decreases with distance to accurately calculate the individual magnitudes. Mastering these concepts will allow for solving the problem effectively.
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Firstly please if you reply don't post the solution, rather the method you would use to get it as I'm trying to learn how to answer this kind of question for an exam.

the problem (quoting my question paper):

the stars S1 and S2 are seen along the same line of sight from Earth. Srat S1 is at a distance of 10pc, the star S2 is at a distance of 100pc. Their apparent flux ratio is known to be (f1/f2)=2.
The combined apparent brightness of both stars seen from Earth is zero magnitudes, i.e m1+2=0.0mag. Determine the individual apparent magnitudes m1 and m2 of the two stars, if they could be resolved.
 
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I'm not familiar with the term "apparent flux ratio", but I'm guessing it means "apparent brightness ratio". If so, the fact that S1 is twice as bright as S2 means that 3 times S2's intensity equals mag. 0. Do you know how to convert "3 times" into a magnitude difference?

Using the same logic, 2/3 of the combined brightness equals S1's brightness. Convert 2/3 (or 3/2; it doesn't matter) into a magnitude difference; the question should be easy from there.
 
You need to know the relation between brightness (or flux) and magnitude (see http://en.wikipedia.org/wiki/Absolute_magnitude)
And you need to know how the brightness of an object decreases with distance.
 
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