Time evolution of a particle captured by the 2:5 MMR with Neptune. Upper panel shows the evolution of the perihelion distance, q, and inclination, i. The middle panel shows the evolution of the argument of perihelion, ω, and the bottom panel presents the resonant angle φ2:5. We notice several dynamical modes like the Kozai+MMR, and the hibernating mode. In the end the particle is in a non-fossilized detached orbit.
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