We study numerically the dynamical system of a two-electron atom with the D
arwin interaction as a model to investigate scale-dependent effects of the
relativistic action-at-a-distance electrodynamics. This dynamical system co
nsists of a small perturbation of the Coulomb dynamics for energies in the
atomic range. The key properties of the Coulomb dynamics are (i) a peculiar
mixed-type phase space with sparse families of stable nonionizing orbits a
nd (ii) scale-invariance symmetry, with all orbits defined by an arbitrary
scale parameter. The combination of this peculiar chaotic dynamics [(i) and
(ii)], with the scale-dependent relativistic corrections (Darwin interacti
on), generates the phenomenon of scale-dependent stability: We find numeric
al evidence that stable nonionizing orbits can exist only for a discrete se
t of resonant energies. The Fourier transform of these nonionizing orbits i
s a set of sharp frequencies. The energies and sharp frequencies of the non
ionizing orbits we study are in the quantum atomic range.