Choose the orientation . To leading order in the radial disturbance, the azimuthal angular frequency is , so
For either orientation the positive frequency ratio is . At , the ratio is : there is one radial oscillation per revolution. The bound Kepler orbit is an ellipse with the force centre at a focus, with one closest and one furthest approach per revolution. Its exact polar coordinates equation is
At , the ratio is : there are two radial oscillations per revolution. The isotropic harmonic oscillator trajectory is an ellipse centred on the force centre. An exact parametrization is
Here repeats twice during one full circuit. The two different placements of the force centre distinguish these ellipses. These are the two all-bound-orbit cases of Bertrand's theorem.
Figure 1.
Nearly circular ellipses: one radial cycle about a focus for the inverse-distance potential, and two about the centre for the quadratic potential
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