How Fast Will the Comet Travel at the Midpoint Between Two Stars?

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The discussion centers on calculating the speed of a comet at the midpoint between two stars in a binary star system, each with the mass of the Sun and separated by 8.00 x 10^11 meters. The initial approach involved equating potential energy and kinetic energy, but the user encountered issues with the calculation of the radius (r). The correct method requires using half the distance between the stars for r, leading to the formula v = sqrt(4(GMsun/r)). The method is fundamentally sound, but clarity on the radius used is crucial for accurate results.

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ok so here's the problem
A binary star system has two stars, each with the same mass as our sun, separated by 8.00 x 10^11 . A comet, far away from both stars is essentially at rest. Slowly but surely, gravity pulls the comet toward the stars. Suppose the comet travels along a straight line that passes through the midpoint between the two stars.
What is the comet's speed at the midpoint?

here's what i tried (but it was wrong)
pe initial(comet)= ke intial = 0
pe final (comet)= ke final= -GMsun/r
since 2 masses --> 2(GMsun/r)


ke = 1/2mvr^2---> v= sqrt(4(GMsun/r))
it says i have the wrong answer...
Is my method completely wrong? What can I do to fix it? Any help is greatly appreciated!:confused:
 
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why do you have 1/2mvr^2 for the kinetic energy? You do end up with the correct expression for v. What did you use for r? r is half the distance between the stars.
 
Method looks fine to me, if r is the distance from midpoint to star.
 

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