With the apsidal origin chosen as specified, G=0. For pϕ=0, rearrangement givesLet u=1/r. Since du/dϕ=−pr/pϕ, the equation is u′=−(u−mk/pϕ2)tanϕ. Its solution, continued through points where the intermediate division fails, isAs printed, e has units of inverse length and is not the usual dimensionless eccentricity. Writing ℓ=pϕ2/(mk) gives the standard form r=ℓ/(1+εcosϕ) with ε=eℓ. The orbit is an ellipse for ∣ε∣<1, parabolic for unit magnitude and hyperbolic for magnitude greater than one on its allowed angular interval. The purely radial case pϕ=0 must be handled separately and is excluded by these divisions.
pr=(rpϕ−pϕmk)tanϕ.
r1=pϕ2mk+ecosϕ.
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