Fig. 5
Distribution of residence times (in Log scale) of 100 000 asteroids in the Hill sphere of the CM (with a null eccentricity) in the planar 2 + 2 body problem for the Eccentric-Neptune case. In a) the CM is in the classical belt (R = 40 AU) and in b) the CM is in the resonance (R = 36.0352 AU). These histograms are linked to the MEGNO maps of Fig. 3.
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