The existence of a fourth constant of motion, beyond rest mass, energy and
axial angular momentum, for a free particle in a Ken spacetime has been sho
wn by Carter through the separability of the Hamilton-Jacobi equation using
oblate spheroidal coordinates. This fourth constant of motion is connected
to a second-rank Stackel-Killing tensor related to the symmetries of the K
en solution; while this mathematical aspect is clear, the physical meaning
of the separation constant is not. In this note we solve this problem, show
ing how the separation constant can be interpreted physically.