Fig. 2.
Variations of the eccentricity and inclination for orbits with different initial inclinations surviving the integration time of 3.4 × 107 yr. The initial eccentricity is 0.04975 for all orbits. There might be many orbits with different initial semi-major axes for each initial inclination. The orange squares indicate orbits whose libration amplitude (Δσ) is larger than 300° while black crosses indicate those which have never left the tadpole region around L4 during the integration time (Δσ < 180°).
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