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A superintegrable Hamiltonian system with degrees of freedom has more than functionally independent integrals of motion, including an integrable set of in involution. At a regular nonzero Hamiltonian vector field, at most independent integral differentials can annihilate the flow. A maximally superintegrable system attains that bound. The three-dimensional Kepler orbit has five independent integrals through energy, angular momentum and the Laplace-Runge-Lenz vector. A closed orbit on one isolated resonance is weaker than maximal superintegrability on an open phase-space region.