The moon's rotation and revolution periods are synchronized due to tidal locking, allowing us to see only one face of the moon. This phenomenon is common among celestial bodies, such as Pluto and Charon, and is caused by the loss of energy in orbiting pairs, leading to synchronized rotations. Tidal friction, influenced by surface liquids, plays a significant role in this process, particularly affecting the moon's rotation due to Earth's greater mass. The discussion also touches on the theoretical aspects of tidal locking, suggesting that perfectly symmetrical and rigid bodies would not experience tidal torques, though this is not practically achievable. Overall, tidal locking is a complex interplay of gravitational forces and the physical characteristics of celestial bodies.