Section 3 review
Linear motion is when an object moves in a particular direction. Circular motion can involve rotating, rolling, or orbiting objects. A centripetal force (directed towards the center of the circle) is required to maintain an object in circular motion. The law of universal gravitation expresses the mutual force of attraction between two masses and is the force that keeps satellites and planets in their orbits.
angular velocity, radian, centripetal force, centripetal acceleration, law of universal gravitation, satellite, orbit

ω= Δθ Δt
v=ωr
a c = v t 2 r
F c = m v 2 r
F=G m 1 m 2 r 2

Review problems and questions

  1. Radians and degrees are related by π rad = 180°. Make the following conversions:
    1. Convert 45° to radians
    2. Convert 0.5236 radians to degrees
    3. Convert 270° to radians
    4. Convert 7.85 radians to degrees
    5. Convert 585° to radians
    6. Draw each one of these angles on a circle. Show
  1. A wheel spins at a rate of 30 revolutions per minute (rpm). What is the angle that a point on the wheel makes in one second? Give your answer in degrees and radians. Show
  1. A race car is moving with a speed of 200 km/h on a circular section of a race track that has a radius of 300 m. The race car and the driver have a mass of 800 kg.
    1. What is the magnitude of the centripetal acceleration felt by the driver?
    2. What is the centripetal force acting on the car? Show
  1. A bicycle moves with a speed of 30 km/h. If the wheels of the bicycle have a radius of 35 cm, what is the angular speed of the wheels?
    Give your answer in rad/sec and degrees/sec. Show
  1. Using the formula for the universal law of gravitation, calculate the force between two spheres of 100 kg each. The distance between the centers of the spheres is 2 m. Show


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