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Unit 9

Circular motion and gravity.

From a ball on a string to the Moon: centripetal force, universal gravitation, orbits and angular momentum.

Before this unit

The unit, lesson by lesson

Lessons

5 lessons · 28 practice questions · about 2 hours

  1. Acceleration towards the centre

    A ball going round a circle at a steady speed is accelerating all the time. Which way, by how much, and how long does one turn take?

    About 25 minutes 6 practice questions

  2. The force that holds it on the circle

    Moving on a circle takes a net force towards the centre, of size m·v²/r. What supplies it, how strong is it, and why is there no force pushing outward?

    About 25 minutes 5 practice questions

  3. Universal gravitation

    Any two masses pull on each other, with the same force, which grows with the masses and weakens with the square of the distance. From the pull between two bodies in the Scene to your own weight.

    About 30 minutes 5 practice questions

  4. Orbits: a fall that never ends

    A satellite is a body that keeps falling and keeps missing the Earth. Gravity is its centripetal force, and from that come its speed, its period, Kepler's third law, and why astronauts float.

    About 30 minutes 6 practice questions

  5. Angular momentum: a skater and a gyroscope

    A spinning body keeps its angular momentum, L = Iω, as long as no torque acts on it: a skater who pulls in her arms and spins faster, the energy she adds, and a gyroscope that circles its stand instead of falling.

    About 25 minutes 6 practice questions

Next unit Oscillations