Assume the velocity-to-momentum Legendre map is locally invertible. Differentiate the Hamiltonian while regarding as independent:
The velocity variations cancel because . Combining the remaining coefficients with the Euler-Lagrange equations gives Hamilton's equations
An ignorable coordinate does not occur explicitly in the Lagrangian, so its conjugate momentum is conserved. For the spherical motion, is ignorable and the Hamiltonian has no explicit time dependence. The two constants are and .
The polar Hamilton equations are
A constant polar angle therefore requires and vanishing of the second right-hand side. For with , this is
The expression must be nonnegative to represent a real momentum. Once it holds, advances uniformly at , so it is also sufficient with those initial data. At the equator the undivided equation instead requires , with any ; dividing by cosine would wrongly discard this special case. The polar coordinate chart itself excludes the poles.

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