A semiclassical propagator is applied to describe the dynamics of circ
ular-orbit wave packets which are initially well localized in three di
mensions. A sum over classical Kepler trajectories for the wave-packet
autocorrelation function is obtained which is extremely accurate well
past the classical regime of the evolution of the wave packet. The no
nclassical nature of the wave-packet evolution at long times is associ
ated with the interference between amplitudes from classical paths at
different energies. The time scale of the wave-packet revivals is rela
ted to the shearing rate of the corresponding classical ensemble.