How Can Luminosity and Temperature Ratios Be Deduced in Binary Star Systems?

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In a particular binary star system, star A has apparent brightness 8x10^(-13) and star B has apparent brightness 2x10^ (-14).

a) Explain how it is possible to deduce that star A has a higher luminosity than star B.

b) The surface area of star B is 10 000 times smaller than that of Star A. Calculate the ratio
surface temperature of star B/ surface temperature of star A

Cheers.
 
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a) Because Star A's temperature may be higher and the body my be larger than Star B.

b) I got no idea how to work it out. I wasn't if i have to find all the unknowns.
 
To solve this, I first used the units to work out that a= m* a/m, i.e. t=z/λ. This would allow you to determine the time duration within an interval section by section and then add this to the previous ones to obtain the age of the respective layer. However, this would require a constant thickness per year for each interval. However, since this is most likely not the case, my next consideration was that the age must be the integral of a 1/λ(z) function, which I cannot model.
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