Image Details
Caption: Figure 8.
Solution of Equation (16). At t = 0 (Γ = 0), the rotation is prograde. Near synchronization, it changes from supersynchronous (y > 0) to subsynchronous (y < 0). Subsequently, it becomes retrograde. Left: the same path as Figure 7. Right: an alternative along a path that drives the solution from domain 0 to domain II, instead of domain I, and eventually to the white domain where the synchronous rotation is unstable. In both cases, Z = −10−3.
© 2026. The Author(s). Published by the American Astronomical Society.