Lunar Craters
Lunar craters are bowl-shaped depressions found on the surface of the Moon. They are formed primarily by the impact of meteoroids, asteroids, and comets colliding with the lunar surface. When these celestial bodies strike, they create a shock wave that excavates material, resulting in a crater. The size of these craters can vary greatly, from small pockmarks to large basins.
Many lunar craters are named after famous scientists, astronomers, and explorers. Some well-known examples include Tycho, a prominent crater with a distinct ray system, and Copernicus, which showcases a well-preserved structure. These craters provide valuable information about the Moon's history and the solar system's evolution.