Universal Gravity
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Universal Gravity Chapter 8
Kepler’s Laws of Planetary Motion • The orbit of each planet is an ellipse with the sun at one focus.
Kepler’s Laws of Planetary Motion 2. The line segment joining a planet to the sun sweeps out equal areas in equal time intervals.
Kepler’s Laws of Planetary Motion The square of the period of revolution of a planet about the sun is proportional to the cube of the semimajor axis of the planet’s elliptical orbit.
r Kepler’s Laws of Planetary Motion T – Period of one orbit r – Distance of the semimajor axis
TA rA Compare Planet A to Planet B TB rB
( ) ) ( 2 3 TA TB rA rB = Compare Planet A to Planet B
Compare Saturn to Earth Find out how long Saturn takes to make one orbit. Earth TE = 1 year rE=1.50X1011m Saturn TS = ? years rS=1.43X1012m (Table 8.1 Page 178 )
( ) 3 ( ) 2 TS TE rS rE = ( ) 3 rS rE = 2 TS TE
( ) ) 3 ( 3 rS rE = 1.43X1012m 1.50X1011m = 2 2 TS TS (1y) TE TS = 29.4 years
Homework: 8-1 Practice Problems: 1-4 Pages: 180-181 Due: 12/13/02
Homework: 8-2 Problems: 41-44 Pages: 195 Lab Write-up Due: 12/16/02