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foreign kids today Im going to show you how to solve for the period of orbit for an object which is in a binary star system you see typically when we have an orbit we might have a central object with something orbiting around it but in a binary system what we have are two different masses which are orbiting around their Mutual center of gravity now what were looking at today is a simplified case of a binary star systems and that were going to say that the two masses are equal to one another and were also going to say that these two masses are in perfectly circular orbits and I know thats not particularly realistic for those of you who are getting into astrodynamics but this is a real typical example that youll see when you first start talking about centripetal forces and noons law of universal gravitation you see the only force acting on either of these masses is the force of gravity between them and just like with any other orbit its this force of gravity thats causing these