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Explore the fascinating mechanics of impacts in our solar system, from the formation of craters on moons and planets to the devastation caused by asteroid collisions with Earth. Discover the energy transformation during impacts, such as a 10-meter rock hitting at 20 km/sec, equating to the energy of 10 Hiroshima bombs. Learn about different types of craters formed by small to large impacts, including simple pit craters and massive multi-ring basins. Delve into how we recognize craters on Earth and their rapid erosion, revealing a history shaped by cosmic events.
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The Solar System • Nine Eight Planets • Over 170,000 catalogued asteroids • ???? Centaurs • ???? KBO’s (including one disgruntled ex-planet) • Millions of Comets
Impact Mechanics • Energy of motion turns into heat • 10-m rock at 20 km/sec = 150 kt = 10 Hiroshima atomic bombs • Energy released in seconds • Impacting object destroyed • Crater 20-30 times diameter of impacting object • Crater is round regardless of approach path
The Impact Process • Atmospheric Entry • Contact-Compression • Penetration – Transient Crater • Excavation • Collapse
Comets and Planetary History • Superposition • Crater Saturation • Crater Degradation
Recognizing Craters on Earth • Craters rapidly destroyed by erosion • Circular geologic structures • Impact melts • Impact breccias • Shock metamorphism • Shatter cones