The Restricted 2+2 Body Problem: Parametric Variation of the Equilibrium States of the Minor Bodies and Their Attracting Regions

Figure 13

Number of points of the attracting subsets 𝑅_𝑆𝑖(𝐿₄),𝑖=1,2, of the inline and the perpendicular equilibria around 𝐿₄ as a fraction of the total number of initial values, for the Sun-Jupiter-binary asteroids system.