Binary star system distance between stars

AI Thread Summary
In a binary star system with a 90-day orbital period and two stars each twice the mass of the Sun, the distance between the stars can be calculated using gravitational and centripetal force equations. The gravitational force between the stars is expressed as GM^2/(2r)^2, where M is the mass of one star and r is the distance from each star to the center of mass. The confusion arises from the use of r versus 2r in the calculations; the stars orbit around a common center of mass located halfway between them. Thus, the correct approach involves recognizing that the gravitational interaction depends on the distance between the stars, which is 2r. Understanding these relationships clarifies the correct equations needed for solving the problem.
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Homework Statement


A binary star system has a period of 90 days. It consists of two equally massed stars each with a mass of twice that of the sun, that rotate like a dumbbell about the center of mass at the midpoint between them. How far apart are these stars?


Homework Equations


F = ma v = 2 pi r/T force of g = GMm/r^2 distance = 2r




The Attempt at a Solution


I set GMm/r^2 = m v^2/r then solve for r and d is 2 r. My problem is that my solution sheet uses force of g = GM^2/(2r)^2 and then force = to M v^2/r I know this has something to do with the fact that we have two stars and therefore, I guess M times M but I am confused... Could someone please explain why the equations used in the solution sheet are the correct ones and why in turn mine are incorrect? Thanks, Frostking
 
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frostking said:

The Attempt at a Solution


I set GMm/r^2 ...my solution sheet uses force of g = GM^2/(2r)^2

You used r^2 where the distance between them is 2r, they are orbiting about a common center of mass.
 
Both stars revolve around their common centre of mass which is halfway between them, at distance r, so the centripetal force is mv2/r, but the other star is 2r distance apart, so the gravitational interaction between the stars is Gm2/(2r)2.

ehild
 
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