The Restricted 2+2 Body Problem: Parametric Variation of the Equilibrium States of the Minor Bodies and Their Attracting Regions
Figure 3
Distribution of the collinear equilibrium solutions in the neighborhood of (a), (b), and (c) Lagrangian points. () (in blue) and () (in red), , for two different cases; (A) Sun-Jupiter-binary asteroids, (B) Earth-Moon-dual satellites.
