T, simple harmonic motion, gravity

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SUMMARY

The discussion focuses on the oscillatory motion of a mass, m, influenced by two other masses positioned symmetrically on the y-axis. The gravitational force acting on mass m is expressed as g = 2Gmx/(x^2 + a^2)^(3/2). Additionally, the conservation of energy principle is applied to determine the velocity of mass m at the origin, starting from rest, by equating potential energy (PE = GMm/(x^2 + a^2)^(1/2)) to kinetic energy (KE).

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kjavia795
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There are two masses both M +a and -a apart with respect to the origin on the y axis. A third mass, m, is x away from the origin. Due to gravity it will oscillate back and forth. What is T
Also, how can I use conservation of energy to find the velocity of the third mass m when it reaches the origin if it started at rest?

so far i got

g=2Gmx/(x^2+a^2)^(3/2)


and for the conservation of energy the PEi has to equal KEf
 
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Hi kjavia, welcome to PF.
Potential energy at any point along the x-axis is given by
PE = GMm/(x^2 + a^2)^1/2.
Equate this to KE at the origin and find v.
 

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