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Chapter 7.3 and 8 Circular and Planetary Motion
Rotational Inertia ,[object Object],[object Object],[object Object],[object Object],[object Object]
Rotational Inertia ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]
Speed and Acceleration in a Circle ,[object Object],[object Object]
Centripetal Notes ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]
Scientists ,[object Object],[object Object],[object Object],[object Object]
Kepler’s Laws of Planetary Motion ,[object Object],[object Object],[object Object]
Formula for Kepler’s Laws T 2 T 1 = 2 r 1 r 2 3
Newton’s Universal Law of Gravitation ,[object Object]
Law of Gravitation F  = G (m 1 ) (m 2 ) / d 2 F = Force in Newtons G = Gravitational Constant M = mass in kg D = distance in meters
Henry Cavendish found the value of G ,[object Object]
Satellite Motion ,[object Object],[object Object],[object Object],[object Object]
Newton’s Variation of  Kepler’s Third Law ,[object Object],[object Object],[object Object]
Newton’s Variation of  Kepler’s Third Law (Derivation) ,[object Object],[object Object],[object Object],[object Object],[object Object]
Satellite orbits ,[object Object]
Gravitational Fields ,[object Object],[object Object]
Gravitational Fields ,[object Object],[object Object],[object Object],[object Object]
Determining the gravity of a planet ,[object Object],[object Object],[object Object],[object Object]
Weightlessness ,[object Object]
Other Gravity Scientist ,[object Object]
Other Gravity Scientist  ,[object Object]

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Physics chapter 7.3 and 8

  • 1. Chapter 7.3 and 8 Circular and Planetary Motion
  • 2.
  • 3.
  • 4.
  • 5.
  • 6.
  • 7.
  • 8. Formula for Kepler’s Laws T 2 T 1 = 2 r 1 r 2 3
  • 9.
  • 10. Law of Gravitation F = G (m 1 ) (m 2 ) / d 2 F = Force in Newtons G = Gravitational Constant M = mass in kg D = distance in meters
  • 11.
  • 12.
  • 13.
  • 14.
  • 15.
  • 16.
  • 17.
  • 18.
  • 19.
  • 20.
  • 21.