Force on a mass by two fixed masses

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The discussion focuses on calculating the gravitational force exerted on a third mass, ##m##, placed along the perpendicular bisector of two identical point masses, each of mass ##M##. The gravitational force is directed inward along the bisector, with a derived magnitude of $$F = \frac {2GMmx}{(x^2+R^2)^\frac{3}{2}}$$. Participants clarify the correct application of gravitational equations and the importance of accurately determining the distance between the masses. There is a specific emphasis on simplifying the expression for cosθ and ensuring the denominator reflects the proper distance in Newton's law of gravity. The conversation highlights common mistakes in the calculations and encourages a clear understanding of the underlying physics principles.
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Homework Statement


Two identical point masses, each of mass ##M##, always remain separated by a distance of ##2R##. A third mass ##m## is then placed a distance ##x## along the perpendicular bisector of the original two masses. Show that the gravitational force on the third mass is directed inward along the perpendicular bisector and has a magnitude of
$$F = \frac {2GMmx}{(x^2+R^2)^\frac{3}{2}}$$

Homework Equations


$$F = G\frac {m_1m_2}{r^2}$$

The Attempt at a Solution


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Am I on the right track? If so, what do I do from here? If not, where did I go wrong?
 
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You're on the right track. In your expression for the force, FM on m, you wrote the denominator as (R2 + x2)1/2. The power of 1/2 is not correct.

You can simplify cosθ. There is no need to write it as cos(tan-1(R/x)). You should be able to "read off" cosθ from one of your triangles in your picture.
 
Why is ##(R^2+x^2)^{1/2}## not correct? Isn't that the distance between ##M## and ##m##?
 
Yes, it's the distance between M and m. But what is the denominator in Newton's law of gravity?
 
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