Image Details
Caption: Figure 1.
Damped, modified Laplace–Lagrange secular solution of a two-planet system with
and
e
2 = 0.1. Three solutions are presented corresponding to the initial conditions
e
1 = 0.1 (blue),
e
1 = 0.03 (red), and
e
1 = 0 (green), with randomly chosen longitudes of perihelia. The black line shows the eccentricity of the outer planet. The
apsidal angles initially circulate, but switch to libration at
t ≈
Q × 6 × 10
5 years. The system reaches a fixed point as the anti-aligned (
g
1) mode decays away completely at
t ≈
Q × 1.3 × 10
6 years. Note that the system loses memory of its initial conditions as it approaches the fixed point.
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