Craters on the moon are primarily formed by the impact of meteoroids, asteroids, and comets colliding with its surface at high speeds. Unlike Earth, the moon lacks a significant atmosphere to shield it from these objects, resulting in a higher frequency of impacts. Over billions of years, this has led to the formation of numerous craters, varying in size and depth, as each impact creates a distinct depression. The moon's geological inactivity has preserved these craters, allowing them to remain visible for millions of years.
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