Fig. 3

Resonant angle of the libration centers (σk) for L4 (top) and L5 (bottom) of Venus from different solutions. The positions of the libration centers for L3 and L1 obtained from the numerical solutions to the equations of motion are also presented in the upper and lower panels, respectively. “SIMP” represents the results calculated from the simplified approximation formulae Eqs. (20) and (21). The results from approximation formulae for L5 are only shown for 0 < β < 0.01 (we insert a window to zoom in) because their deviations from the numerical solutions are too large for β > 0.01.
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