The uneven cratering of the Moon's surface is attributed to the fact that one side is more heavily cratered than the other, with the Earth providing some protection to the side that faces us. The side facing Earth has experienced significant volcanic activity, leading to the formation of large Maria, while the far side lacks these features. Despite the Moon being closer to Earth in the past, it could not have been shielded from impacts without breaking apart due to gravitational forces. Additionally, a parallel is drawn to Earth, where the Pacific Ocean represents a similar geological feature to the Moon's Maria. This phenomenon raises intriguing questions about the Moon's history and the dynamics of celestial impacts.