1Angular momentum of a particle
Angular momentum is the momentum of turning, measured about a point (or an axis).
Even a body moving in a straight line has angular momentum about a point off its path. A 2 kg ball at 5 m/s passing 3 m from O: as it moves, and change, but stays 3 m, so kg m²/s stays constant.
Example: 0.5 kg at 8 m/s, 2 m from an axis: kg m²/s.
2L = Iω for a spinning body
Each bit of a spinning body moves at , so its angular momentum is . Adding all the bits:
| Moving in a line | Turning |
|---|---|
| no outside force: kept | no outside torque: kept |
| kg m/s | kg m²/s |
3Torque changes angular momentum
4Conservation of angular momentum
If the net outside torque is zero, and the angular momentum stays constant:
Forces inside the system (muscles, friction between parts) can change , but they come in pairs whose torques cancel, so they cannot change .
5Energy is not conserved
With fixed, a smaller means more kinetic energy: . Pulling the weights from 1 m to 0.5 m (I 8 → 5, ω 0.5 → 0.8 rad/s) raises the kinetic energy from 1 J to 1.6 J. The extra energy is the work the muscles do pulling the weights inward.
6Joining up
7Orbits and real life
The Sun's pull on a planet points straight at the Sun, so it has no torque about the Sun: the planet's angular momentum is kept. Near the Sun it moves fast, far away slowly, and it sweeps out equal areas in equal times (Kepler's second law).
A comet at 50 km/s, 1 unit from the Sun, moves at 10 km/s at 5 units. A spacecraft that fires its engine along its path does feel a torque about the Earth or Sun, so its changes during the burn; afterwards, on its new orbit, again. For example, 8.2 km/s at perigee 7000 km gives about 5.7 km/s at apogee 10 000 km.
Summary
Key ideas
- Angular momentum is the momentum of turning: L = r × p, size mvr⊥.
- A particle moving in a straight line has constant L about any point.
- For a spinning body L = Iω, the twin of p = mv.
- Torque is the rate of change of angular momentum; a steady torque gives ΔL = τΔt.
- With no outside torque, L is conserved: I₁ω₁ = I₂ω₂.
- Internal forces can change I but not L.
- KE = L²/2I: pulling in raises the kinetic energy; joining up loses some.
- Opposite spins have opposite signs.
- About a pivot, L is kept in a collision even though momentum is not.
- Planets keep L: v₁r₁ = v₂r₂, equal areas in equal times.
Every equation
- Particle
- Size
- Spinning body
- Torque
- Angular impulse
- Conservation
- Kinetic energy
- KE when I changes
- Joining up
- Ball sticking to a pivoted rod
- Orbit ends