With the apsidal origin chosen as specified, . For , rearrangement gives
Let . Since , the equation is . Its solution, continued through points where the intermediate division fails, is
As printed, has units of inverse length and is not the usual dimensionless eccentricity. Writing gives the standard form with . The orbit is an ellipse for , parabolic for unit magnitude and hyperbolic for magnitude greater than one on its allowed angular interval. The purely radial case must be handled separately and is excluded by these divisions.

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