2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/1884Our numerical simulations of the Edgeworth-Kuiper belt objects gravitationally scattered by the four giant planets accounting for mean motion resonances reveal numerous resonant gaps in the distribution of the scattered population.2 pages with one encapsulated Figure. Highlights of Astronomy, Joint Discussion 4. Eds. A. Lemaitre and H. Rickman (in press)Astrophysicstext