The near side of the Moon is always visible from Earth due to tidal locking, a phenomenon where the Moon's rotation period matches its orbital period around Earth. This synchronization results from tidal friction, which slows the Moon's rotation over time, allowing it to settle into a stable configuration where the same side faces Earth. The gravitational interaction between the Earth and the Moon creates tidal bulges, which exert torque that maintains this alignment. As a result, the Moon's surface features, such as mountains and highlands, contribute to this gravitational pull. Ultimately, the Earth and Moon will continue to evolve toward a state where both are tidally locked to each other, similar to other celestial bodies in the solar system.