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Table 2

Parameters of the two numerical simulations.

# Ω x y ε δ
0 4 × 10−12 1 1 2 × 10−4 −5.51
1 4 × 10−12 1/10 100 2 × 10−4 −5.46

Notes. In this table, the chosen value of δ is that of the maximum of the region where all the real parts are negative, ensuring that the system crosses the whole linearly stable region. The rotations of the planets are initially synchronised and both sets of parameters verify m3/m0 = 10−4, and ā = 0.02 AU. System 1 is the system that was used for all the figures in Sects. 2 and 3.

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