There are several kinds of binaries:
With a double-lined binary it is possible to measure masses of
the stars to within a factor that depends on the inclination
of the orbit with respect to the line of sight.
Measure the masses for as many stars as you can find in these systems and discover the Mass-Luminosity relation for main-sequence stars.
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There is a pretty "steep" relationship between Mass and Luminosity in the sense that more massive stars are more luminous, thus
The Main-Sequence in the H-R Diagram is a Mass Sequence!
For each position along the main sequence there is a corresponding stellar mass: