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Lunar geography

Lunar geography refers to the study of the Moon’s surface features and landscape. The Moon is marked by craters, formed by impacts from meteoroids, and large dark plains called "maria," which are basaltic lava flows from ancient volcanic activity. It also has highlands, which are brighter, mountainous regions. The lack of atmosphere means there are no weathering processes, preserving these features for billions of years. Understanding lunar geography helps scientists study the Moon's geology, history, and potential for future exploration or habitation.

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    Lunar geography refers to the study of the Moon's surface features and landscape. It includes the vast plains known as "maria," formed by ancient volcanic activity, and the highlands, which are older, more cratered regions. Impact craters from asteroid collisions dot the surface, varying in size and age. The Moon also has mountains and valleys, with notable features like the lunar poles, where permanently shadowed areas may hold ice. Understanding lunar geography helps scientists learn about the Moon's history, its formation, and its potential resources for future exploration.