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Problem 11

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Title: Problem 11 Author: xrg Last modified by: Hans Schuessler Created Date: 4/18/2005 6:05:13 AM Document presentation format: On-screen Show Company – PowerPoint PPT presentation

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Title: Problem 11


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Chapter 12 Gravitation
Newtons 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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Keplers 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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