For a particle constrained to , the kinetic energy and potential energy areIn the stipulated gentle-surface small-slope approximation, the second kinetic term is higher order. The leading Euler-Lagrange equations for therefore give the small-slope particle motion on a height graph:This is also the small-slope component of gravity along the surface, with . Geometric acceleration terms must remain negligible at the speeds considered; the approximation is not asserted for arbitrarily fast motion on a sharply curved surface.
For , the equations are , . If , put . For arbitrary initial data the motion isIt is simple harmonic motion across the trough and uniform motion along it. If , both coordinates move uniformly; if , the same formula uses and instead.
For the radial height profile, is positive for , zero at , and negative for . Its derivative is , so the minimum is . It diverges to positive infinity as and tends to from below as . The requested profile sketch is shown below.
The equations in polar coordinates in the planar approximation areMultiplying the second equation by gives . Thus the specific angular momentum is conserved, andAt release with negligible radial velocity, the initial specific kinetic energy is indeedIt is not the total energy. Put . The conserved specific total energy and effective potential areThe radial turning points for an inverse-square height well follow fromAs a function of , this expression tends to at zero, has its maximum at , and tends to at infinity. Only regions where it is nonnegative are dynamically accessible. If , there are two positive turning radii,and the radial coordinate is confined between them. They merge at , the circular orbit. If , the particle escapes to arbitrarily large radius with radial speed tending to zero; if , it escapes with positive limiting radial speed. Consequently the bounded-orbit condition, including the circular case, isThe circular release is at . For , the release point is the smaller turning radius; for , it is the larger one. These statements concern the prescribed planar small-slope model. The literal surface is steep near its central singularity, so that approximation must be valid along the particular orbit under consideration.
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