What can result from tidal forces experienced by celestial bodies?

Tidal forces arise from the gravitational interaction between two bodies, such as a planet and its moon, or a star and its companion. These forces create variations in gravity across the body, leading to stretching and deformation. For instance, the gravitational pull of the Earth on the Moon results in the Moon becoming slightly elongated rather than perfectly spherical. Similarly, the tides on Earth caused by the Moon's gravity illustrate how these forces can lead to fluctuations in shape and volume, creating bulges in water bodies.

In contrast, the creation of binary star systems involves the pairing of two stars due to their mutual gravitational attraction but does not inherently result from tidal forces acting on them. Stabilization of planetary orbits typically relates more to gravitational dynamics rather than tidal influences. Formation of supernova remnants is a process that occurs after a massive star has exploded, which is unrelated to tidal forces but rather the processes of stellar evolution.

Thus, the most direct and relevant consequence of tidal forces is the deformation and stretching that occurs as one celestial body exerts gravitational influence over another.