Fig. 11

Evolution in time of the inclination i (top panel) and the eccentricity e (bottom panel) of a particular Type-F particle. The system is composed of a Jupiter-mass planet with semimajor axis a = 9.9 au, and eccentricity e = 0.95 and a small body reservoir whose members are all Type-F particles. Moreover, the particles undergo large amplitude of oscillation in eccentricity. The post IE orbital parameters of this particle are a1 = 32 au, e1 = 0.05, i1 = 33.1°, ω1 = 170.9°, Ω1 = 132°.
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