An impact crater is an approximately circular depression in the surface of a planet, moon or other solid body in the Solar System, formed by the hypervelocity impact of a smaller body with the surface. In contrast to volcanic craters, which result from explosion or internal collapse, impact craters typically have raised rims and floors that are lower in elevation than the surrounding terrain. Impact craters range from small, simple, bowl-shaped depressions to large, complex, multi-ringed impact basins. Meteor Crater is perhaps the best-known example of a small impact crater on the Earth.
Impact craters are the dominant geographic features on many solid Solar System objects including the Moon, Mercury, Callisto, Ganymede and most small moons and asteroids. On other planets and moons that experience more active surface geological processes, such as Earth, Venus, Mars, Europa, Io and Titan, visible impact craters are less common because they become eroded, buried or transformed by tectonics over time. Where such processes have destroyed most of the original crater topography, the terms impact structure or astrobleme are more commonly used. In early literature, before the significance of impact cratering was widely recognised, the terms cryptoexplosion or cryptovolcanic structure were often used to describe what are now recognized as impact-related features on Earth.
The cratering records of very old surfaces, such as Mercury, the Moon, and the southern highlands of Mars, record a period of intense early bombardment in the inner Solar System around 3.9 billion years ago. Since that time, the rate of crater production on Earth has been considerably lower, but it is appreciable nonetheless; Earth experiences from one to three impacts large enough to produce a 20 km diameter crater about once every million years on average. This indicates that there should be far more relatively young craters on the planet than have been discovered so far. The cratering rate in the inner solar system fluctuates as a consequence of collisions in the asteroid belt that create a family of fragments that are often sent cascading into the inner solar system. Formed in a collision 160 million years ago, the Baptistina family of asteroids is thought to have caused a large spike in the impact rate, perhaps causing the Chicxulub impact that may have triggered the extinction of the dinosaurs 66 million years ago. Note that the rate of impact cratering in the outer Solar System could be different from the inner Solar System.
Although the EarthÕs active surface processes quickly destroy the impact record, about 170 terrestrial impact craters have been identified.
World's first mountaintop impact crater discovered in northeastern China Live Science - September 15, 2023
A nearly mile-wide (1.6 kilometer) divot in a Chinese mountaintop is actually an impact crater from a long-ago meteorite landing. The newly discovered crater, located in northeastern China not far from the North Korean border, is the first confirmed mountaintop crater on Earth. Researchers aren't sure when the impact happened, but it left a circular depression and split the mountaintop into two peaks, known as Front Baijifeng and Rear Baijifeng. The mountain peaks are littered with rock fragments known locally as "celestial stone," which turns out to be a scientifically accurate moniker.
Earth Oldest Impact Craters Are Disappearing Science Alert - August 2, 2023
The earliest impact scars from asteroids that bombarded Earth's surface may be lost forever to the ravages of time. According to a new analysis, there's a reason scientists have been unable to find any craters older than about 2 billion years. The constant erosion and geological processes on Earth have likely erased them from the surface completely, leaving behind only the barest traces, such as high-pressure minerals and melted rock.
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