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Minor Bodies of the Solar System Chapter 7
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Kepler’s Laws 1. Planets orbit the sun in elliptical orbits with the sun at one focus of the ellipse
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Keper’s Second Law As a planet moves in its orbit, a line connecting the planet to the sun sweeps out equal areas in equal times
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Kepler’s Third Law P 2 = a 3 (provided the period is in Earth years and the semi-major axis in astronomical units)
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The Main Asteroid Belt
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Ceres: Largest Main Belt Asteroids
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Gaspra and Ida (and Dactyl)
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Mathilde and Eros
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NEAR close-ups of Eros
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Resonances in the Asteroid Belt
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Main Asteroid Types C type: carbonaceous, low albedo S type: stony or stony-metallic, redder E type: high albedo, magnesium silicate D type: very dark and red M type: mostly iron and nickel E, S, and M types may be fragments from a larger body that underwent differentiation
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Asteroid Light Curves Antigone
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Kuiper Belt and Oort Cloud
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Pluto: Planet or Kuiper Belt Object
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Pluto
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Sedna
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Comets: Dirty Snowballs
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SOHO Comets
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Comets Hyakutake and Hale-Bopp
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Impact with Comet Tempel 1 at 23,000 mph on July 4, 2005
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Shoemaker Levy 9
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Hits Jupiter July 1994
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Meteors and Meteorites
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Meteor Showers
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