Equations · equation

Angular Momentum

Mechanics · 1775

Equation
L = r × p = Iω; dL/dt = τ
Field
Mechanics
Symbols
L angular momentum · r position from the axis · p linear momentum · I moment of inertia · ω angular velocity · τ net torque
Year
1775

Significance

What a spinning or orbiting body keeps unless a torque acts on it. Kepler's second law — equal areas in equal times — is its conservation for a planet, seen eighty years before Newton explained why. It is why a gyroscope holds its axis, why a collapsing star spins up into a pulsar, and why a turbine's blades are shaped to change the working fluid's angular momentum as it passes.

Machines

Requires

Required By

Referenced by

equation
machine

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From the Equations database in Notion, last edited 2026-08-18. This page is the row, rendered by the build; nothing on it is written by hand.