Three uniform spheres of mass M and radius R each are kept in such a way that each touches the other two. The magnitude of the gravitational force on any of the sphere due to the other two sphere is
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3^(1÷2)GM^2/(4(R^2))
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Answer:
f1=f2=f3
Gm^[2/4r]^2 = 4gm^/3r
fr=2fcosn/2 = root3 Gm^2/4R^2
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