Inner part of the outer debris disk revealed by ﹩\simeq 3.3\times {10}^{6}\langle Y\rangle ﹩ stable orbits found in the whole debris disk simulation, illustrated as a snapshot of astrocentric coordinates (x, y) and osculating orbital eccentricities e₀ of these orbits at the initial epoch, color-coded and labeled in the top bar. The initial positions of planets are marked with filled circles. Gray rings illustrate their orbits integrated in a separate run for 10 Myr.