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Lunar Geology

Lunar geology is the study of the Moon's physical structure and composition. It involves examining the Moon's surface features, such as craters, mountains, and plains, to understand its history and formation. Scientists analyze lunar rocks and soil, collected during missions like Apollo, to learn about volcanic activity and impacts from asteroids. The Moon's geological history reveals important insights about the early solar system and the processes that shape celestial bodies. Understanding lunar geology is crucial for future exploration and potential colonization, as it helps inform resource utilization and the development of sustainable habitats.

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    Lunar geology is the study of the Moon's composition, structure, and processes. It explores features like craters, mountains, and volcanic plains, revealing details about the Moon's history and the solar system's formation. The Moon’s surface is covered in a layer of dust and small rocks called regolith, formed by impacts from meteoroids. Unlike Earth, the Moon lacks water and atmosphere, affecting its geological activity. By analyzing lunar rocks and soil, scientists learn about volcanic activity, impact events, and the Moon's evolution, contributing to our understanding of planetary processes beyond Earth.