Motion Equation Central Force
The basic equation of motion of a particle moving under the influence of a central force F = Fr er is
where, acceleration a = ar er of the particle. We shall now solve the above equation for the spherically symmetric inverse square force:
Fr = – C/r2 (C > 0)
Our task is to find the trajectory of the particle, i.e. a relation between r and θ. (Remember, the motion of the particle is confined in a plane and its position is given by co-ordinates r and θ at any time.) To do that, we use the fact that angular momentum of the particle is a constant of motion:
If we introduce the variable u = 1/r. Hence, we get
Substituting above relation, we find
Taking, Fr = – Cu2, we get the simple relation,
The above can be rewritten as
which is the familiar equation of simple harmonic motion; its solution is,
(u – A) = B cos (θ – θ0)
where, B and θ0 are constants of integration.
Thus we get the equation of the trajectory as,
U = 1/r = A + B cos (θ – θ0)
or, p/r = 1 + e cos (θ – θ0)
where, 1/A, and e = B/A are constants of motion.
It is the standard equation of the conic section, i.e. the equation of the curve formed by the section of a cone by a plane. The constants p is called the orbital parameter and e is called eccentricity. The conic section may be an ellipse (e < 1), a circle (e = 0), a parabola (e = 1), or a hyperbola (e > 1). That is, in general, the path of a particle under an inverse-square force produced by a fixed source (center of force) in space could be bounded (ellipse or circle), or unbounded (parabola or hyperbola) depending upon the value of e.
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