The moon is receding from the Earth at approximately 3.8 cm per year due to tidal torques, but this does not affect the length of the year since the Earth's distance from the sun remains unchanged. While the moon's retreat does slightly alter the length of the day, the impact of tidal interactions with the sun is more significant. Discussions highlight that the gravitational dynamics of the Earth-moon-sun system are complex, but the consensus is that the changes in orbital periods are negligible. Tidal forces primarily affect the Earth's rotation, leading to a gradual slowdown, but the overall effect on the Earth's orbit is minimal. Understanding these interactions requires careful consideration of various gravitational influences and their relative magnitudes.