The Moon is tidally locked to the Earth, meaning it always shows the same face due to the gravitational forces acting on it, which are proportional to 1/R3. The proximity of the Moon to Earth, its smaller size, and its irregular shape contribute to a much shorter tidal lock time compared to the Earth’s relationship with the Sun. While no planets are tidally locked, most close-in moons are, with Hyperion being a notable exception. The discussion raises the question of whether all orbiting bodies will eventually become tidally locked given sufficient time. Understanding these dynamics highlights the complex interactions between celestial bodies.