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

<table>Regions of stability (red) and instability (green) for the perpendicular equilibrium points. Points A and B show, respectively, the Sun-Jupiter-binary asteroids system and the Earth-Moon-dual satellites one.</table>

International Scholarly Research Notices

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Figure 8

Figure 8: The Restricted 2+2 Body Problem: Parametric Variation of the Equilibrium States of the Minor Bodies and Their Attracting Regions 