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Appendix B: Complementary tables and figures

Figure B.1 is similar to Fig. 3, but now extended to 100 Myr. We note that the general behaviour of the elements after 5 or 10 Myr is almost unchanged.

Table B.1 refers to the non-successful case, that is, at least one of the current regular satellite is lost during migration. In the table of this Appendix, when a given satellite experiences a collision with another satellite, in the column of the given satellite we indicate this with M, A, U, T, O, and si (the name of the participant of the collision). On the other hand, if the participant is a planetesimal, we indicate it with m/d, where m is the mass ( × 10^-9 M_⊙) and d is the diameter (in km) of the planetesimal.

	Fig. B.1 Similar to Fig. 3 but time extended to 100 Myr. Here we also show the evolution of the perihelion (q) and aphelion (Q) of the planets during migration.
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© ESO, 2011