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Fig. 10

image

Orbital evolution of the synthetic family (black circles) compared to the orbital distribution of the observed members of the actual Euphrosyne family (blue crosses) in the proper (ap, ep) plane. Dotted vertical lines are centers of several two-body and three-body mean-motion resonances located in the region of interest. The red dashed curve shows the approximate position of the ν6 secular resonance (adapted from Carruba et al. 2014; Milani et al. 2019). Individual snapshots, labeled with a corresponding integration time t, map the progress of our N-body simulation. They depict a compact family, the “best-fit” solution, and a dynamically dispersed family.

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