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Fig. 5


Snapshots in time from a coplanar system (2D-POP, 2_09) with initially moderate eccentricities. At 40 Myr, three terrestrial planets are formed and (due to gravitational interactions) the outer giant planet is ejected from the system at ~47 Myr. Only two -mass planets survive the destabilisation phase, and remain on eccentric and inclined orbits until the end of the simulation. Formatted as in Fig. 3.

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