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I have a problem with one detail in quite a simple exercise. It goes like this. Two stars are revolving in circular orbits around their common center of mass. The masses are given and it is told that their mutual distance remains constant (this distance also given). The period is asked; with the above mentioned assumption they have the same periods.
Now this is not hard to do and I have no problems with solving the exercise. I just can't see why their mutual distance remains constant. I suspect it follows from a conservation law (angular momentum?). Help would be appreciated as always :-).