Determining the individual magnitudes of two stars

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SUMMARY

The discussion focuses on determining the individual apparent magnitudes of two stars, S1 and S2, based on their distances and apparent flux ratio. Star S1 is located at 10 parsecs, while star S2 is at 100 parsecs, with an apparent flux ratio of (f1/f2) = 2. The combined apparent brightness of both stars is zero magnitudes, leading to the conclusion that the individual magnitudes can be calculated using the relationship between brightness and magnitude, specifically applying the formula for magnitude difference based on flux ratios.

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Mike89
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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.
 

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