When an object is positioned between two large masses with significant gravitational pull, the gravitational forces can balance out, preventing the object from being violently pulled apart. Tidal forces, which arise from the varying gravitational pull on different parts of an object, become significant when the objects are close together, particularly within the Roche limit. An example of a stable position is the L1 Lagrangian point, where an object experiences balanced gravitational forces and is unlikely to break apart. In a hypothetical hollow planet, an object at the center would not feel any gravitational force from the surrounding mass, effectively allowing it to "float." Overall, the gravitational interactions depend on the distances and configurations of the masses involved.