A special case of the → three-body problem in which the → mass of one of the bodies is negligible compared to that of
the two others. If the relative motion of the two massive components is a circle,
the situation is referred to as the
→ circular restricted three-body problem.
An example would be a space probe moving in the
→ gravitational fields of the → Earth and the → Moon,
which revolve very nearly in circles about their common
→ center of mass.