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Universal Gravitation
Chapter 8 Universal Gravitation
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Drill: Calculate ac & Fc of a 25 kg ball rotation at the end of a 4.0 m rope at revolutions per second.
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Planetary Motion Galileo Tycho Brahe Johannes Kepler Isaac Newton
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Kepler’s Laws of Planetary Motion
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1) The paths of planets are ellipses, with the sun as one focus
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2) An imaginary line from the sun to any planet sweeps out equal areas in equal time intervals. Planets move faster when closer to the sun
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3) The square of the ratio of the periods of any two planets = the cube of the ratio of their orbits average radii
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( )2=( )3 TA rA TB rB
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Drill: Planet. Orbital. Period Name. Rad. (km). (s) Mo 2. 0 x 108. 4
Drill: Planet Orbital Period Name Rad. (km) (s) Mo x x 106 Smit x ? Solve for ?
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Drill: Planet. Orbital. Period Name. Rad. (km). (s) Smo 2. 0 x 108. 4
Drill: Planet Orbital Period Name Rad. (km) (s) Smo x x 106 Mit ? x 109 Solve for ?
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Universal Gravitation
Isaac Newton Henry Cavendish Michael Faraday Albert Einstein
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An attractive force that exist between all objects
Gravitational Force An attractive force that exist between all objects
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Found to directly proportioned to the masses of the two objects
Gravitational Force Found to directly proportioned to the masses of the two objects
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Gravitational Force Fg m
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Found to inversely proportioned to the distance2 between two objects
Gravitational Force Found to inversely proportioned to the distance2 between two objects
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Gravitational Force 1 d2 Fg
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Universal Law of Gravitation mAmB d2 Fg = G
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Gravitational Constant
6.67 x Nm2/kg2
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Calculate the gravitational force between 5. 0 Mg & 6
Calculate the gravitational force between 5.0 Mg & 6.0 kg objects whose centers are 3.0 mm apart:
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The gravitational force between 6. 0 Mg & 50. 0 kg objects is 2
The gravitational force between 6.0 Mg & 50.0 kg objects is 2.22 x 10-2 N. Calculate the distance between them.
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mEmo d2 Fg = G Fg = mog
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Thus: mEmo d2 mog = G
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mEmo d2 mog = G d = r, thus
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GmE r2 g =
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GmE r2 g = or
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Mass of the Earth gr2 G mE =
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Drill: rE = 6.37 x 103 km Solve for the mass of the Earth:
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Centripetal Force m4p2r T2 Fc =
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Fg = Fc msmp mp4p2r r T2 G =
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msmp mp4p2r r T2 G =
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ms p2r r T2 G =
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T2ms p2r3 G =
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Therefore ( ) 4p2 Gms T2 = r3
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Kepler’s Constant for Solar System
( ) 4p2 Gms k =
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Earth’s mean orbital radius is 1. 50 x 107 km while its period 365
Earth’s mean orbital radius is 1.50 x 107 km while its period days. Calculate the Sun’s orbital constant in m3/s2:
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The moon’s mean orbital radius is 4
The moon’s mean orbital radius is 4.00 x 105 km while its period 28 days. Calculate the Earth’s orbital constant in m3/s2:
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or ( ) 4p2 Gms T2 = r3
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Mass of the Sun 4p2r3 GT2 ms =
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mEmo d2 Fg = G Fc = mov2/r
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Thus: mEmo mov2 r r G =
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mEmo mov2 r r G = Thus:
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mE v2 r G = Take sq. rt. of both sides
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Orbital Velocity GmE r v =
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v = (g)r
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Calculate the velocity of a object orbiting at 50. 0 m around a 5
Calculate the velocity of a object orbiting at 50.0 m around a 5.0 x 106 Mg object
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r3 GmE Ts= 2p
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Calculate the period of a object orbiting at 50. 0 m around a 5
Calculate the period of a object orbiting at 50.0 m around a 5.0 x 106 Mg object
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( ) rE d a = g
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Calculate the velocity of a satelite orbiting at 620 km above the Earth’s surface:
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The space in which the force of gravity is apparent
Gravitational Field The space in which the force of gravity is apparent
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Measure of Mass Use a balance
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Inertial Mass minertial = Fnet/a
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Gravitational Mass Fgr2 GmE mg =
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Warped Space ?
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Review
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List Kepler’s Laws of Planetary Motion
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What is the formula for Kepler’s 3rd Law
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Planet. Orbital. Period Name. Radius (km). (s) Two 2. 0 x 108. 4
Planet Orbital Period Name Radius (km) (s) Two x x 106 Twit ? x 109 Solve for ?
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What is the formula for the Universal Law of Gravitation
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The masses of Earth & moon are 5. 98 x 1024 kg & 1
The masses of Earth & moon are 5.98 x 1024 kg & 1.0 x 1024 kg respectively. The average radius of the moon’s orbit is 4.0 x 106 km. Calculate the force of gravity between the Earth & the moon.
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Orbital Velocity GmE r v =
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Calculate the velocity of the moon.
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Calculate the ac & Fc of a merry-go-round with a radius of 50
Calculate the ac & Fc of a merry-go-round with a radius of 50.0 m spinning at 1 revolution every 4 seconds.
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A car is driven off a 2. 0 km cliff at 180 km /hr
A car is driven off a 2.0 km cliff at 180 km /hr. Calculate: tair, maximum vV, & dH:
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A catapult launches a 250 kg rock at 100. 0 m/s at 37o from horizontal
A catapult launches a 250 kg rock at m/s at 37o from horizontal. Calculate: tup, dV, tair, & dH :
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Drill: A 3200 kg carousel with a diameter of 20.0 m is spinning at 1 revolution every 5 seconds. Calculate: ac & Fc
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Important Formulas
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( )2=( )3 Orbital Formula TA rA TB rB
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Universal Law of Gravitation mAmB d2 Fg = G
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Orbital Velocity GmE r v =
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Orbital Velocity v = (g)r
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