Orbital evolution of the fictitious Trojans indicated in Fig. 3 for the model Ve2Sa (red) and Ve2Ne (black). From left to right, the three panels corresponding to the magenta, black, and red stars are of the initial conditions of (a₀, i₀)=(0.9990, 48 ° ), (0.9990, 50 ° ),  and (0.9982, 53 ° ). We illustrate the temporal evolution of e, Δϖ₅, and i for both models, Δϖ₇, Δϖ₈, and ω for the model Ve2Ne only and Δϖ₂, Δϖ₃, ΔΩ₂, and ΔΩ₃ for the model Ve2Sa only. The vertical dashed lines in the bottom plots of each panel indicate the lifespans of the orbits being in the 1:1 MMR.