Giant Moon Crater
An overhead view reveals a massive celestial impact crater featuring a raised outer rim, a broad floor, and a central peak.
A4 format (landscape), black outlines on a white background · for home and classroom use
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Topography of a Lunar Crater
Impact craters are formed when high-speed space objects strike a rocky celestial body like a moon or planet. The force of collision excavates a circular depression with a thick elevated rim and a flat inner floor, often leaving a central mound formed by rebounding rock crust.
How Impact Craters Preserve History
Because airless moons lack wind and liquid water erosion, impact craters can remain almost completely unchanged for billions of years. Studying the size and density of craters allows planetary scientists to determine the relative age of different regions on a celestial body. Larger meteorites generate enough heat upon impact to melt rock and create central uplift peaks.
Real Colors of a Lunar Crater
- Outer crater rim: light gray to off-white pulverized rock
- Crater floor basin: dark gray or dusty charcoal
- Central peak mound: pale gray or silver-gray mineral rock
- Surrounding lunar surface: dark slate, charcoal gray, or ash gray