The Jacobi constant is a conserved quantity for the circular restricted three-body problem. In barycentric coordinates rotating at constant angular frequency , defineThe equation of motion in a rotating frame is . Taking its dot product with proves : the Coriolis force does no work.
Only positions satisfying are accessible. The boundary gives a zero-velocity surface; openings near Lagrange points allow transit between regions but do not force it. Ordinary inertial-frame energy can change even while remains constant.[ref]
Introduction to Celestial Mechanics by Richard Fitzpatrick. Online “Jacobi integral”, equations (9.10)–(9.15): conserved combination and nonconservation of inertial energy
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