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This comprehensive overview explores the complex phenomena of impacts within our solar system, covering the dynamics of nine planets, over 170,000 catalogued asteroids, comets, and Centaurs. It delves into the mechanics of impact, illustrating how the energy of motion converts to destructive heat, leading to crater formation. The process of atmospheric entry, contact-compression, and excavation is examined, alongside the identification of craters on Earth, including erosion's effect. Notable impact sites are discussed, showcasing evidence and computer simulations that enhance our understanding of these 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