Why Is 2r Used in Calculating the Masses in Plaskett's Binary System?

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SUMMARY

The discussion centers on the application of Kepler's laws to calculate the masses of two stars in Plaskett's binary system, which orbit each other at a velocity of 220 km/s with a period of 14.4 days. The correct formula for calculating the gravitational force involves using the distance between the two stars, denoted as 2r, rather than just r. This distinction is crucial because it reflects the relationship between the stars and their center of mass, leading to the equation GMm/(2r)² = mv²/r for accurate mass determination.

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hey
i've been having trouble understanding a part in this question. i'll just map out the basics to the question: 2 stars with a velocity of 220km/s are orbiting at equal distance. the masses of the stars are equal. period = 14.4 days it asks to find the mass of each star.

i understand that u can use kepler's law to get the answer.

GMm/r2 = mv2/r

-which is what i used to come up with my answer seeing that i found the mass relative to a center mass. but according to the solution it's suppose to be:

GMm/(2r)2 = mv2/r

my question is, why is r denoted 2r in order to arrive at a correct answer?
 
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On the left hand side, you use the distance between the 2 stars.

On the right hand side, you use the distance from a star to the center of the circular orbit.
 

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