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Published byUtami Darmadi Modified over 6 years ago
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Chapter 12: Gravitation Newton’s Law of Gravitation
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Gravitational attraction
Note: Two particles of different mass exert equally strong gravitational force on each other
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Gravitational Forces (I)
MM MM ME FG = G r 2 ‘‘Attractive Force” ME
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Cavendish balance Cavendish(1798) announced that he has weighted the earth
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Average Density of the Earth
g = 9.80 m/s2 RE = 6.37 x 106 m ME = 5.96 x 1024 kg rE = 5.50 x 103 kg/m3 = 5.50 g/cm3 ~ 2 x rRock ???
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The gravitational force is conservative
Note: Work done is Path independent!
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Gravitational potential energy
Note: The gravitational potential is zero at infinity
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Projectile
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Projectile
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Circular orbit
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Kepler’s Laws Each planet moves in an elliptical orbit, with the sun at one focus of the ellipse A line from the sun to a given planet sweeps out equal areas in equal times. 3. The periods of the planets are proportional to the 3/2 powers of the major axis lengths of their orbits.
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Geometry of an ellipse
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Elliptical orbit
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