Conservation of angular momentum Created 2026-09-28 Updated 2026-10-14
Conservation of angular momentum says that total angular momentum stays fixed when the net external torque about the chosen fixed inertial origin vanishes. Individual angular momenta and angular velocities can change. The radius change at constant angular momentum below makes this distinction visible: pulling two rotating point masses inward lowers the moment of inertia, raises the angular velocity, and supplies work that increases the kinetic energy.
Figure 1.
Pulling two point masses inward preserves angular momentum and adds three joules of kinetic energy
. Details.
Follow the same constant-mass point masses throughout, in an inertial frame, with all positions measured from a fixed origin . If the internal pair forces are opposite and central, meaning directed along each pair's separation, then
Thus zero net external torque throughout an interval implies constant total angular momentum throughout that interval. A vanishing external torque component, such as , conserves the corresponding even when the other components change. This is the balance law for a fixed collection; angular-momentum flux must also be accounted for when matter crosses its boundary. [ref]
The central qualification is essential. Write for the internal force on member from member . Under Newton's third law, , but the sum of their torques is
This vanishes when is parallel to . Equal-and-opposite forces alone do not suffice: two opposite transverse forces with separated lines of action form a couple with nonzero torque. Cancellation of the internal pair torques, together with Newton's second law, proves the total balance above.
For one point mass under a central force about , gives . The force may still change the speed and kinetic energy; its zero torque preserves angular momentum. With nonzero , keeps the motion in a fixed plane. Choosing the axis perpendicular to that plane, governs its angular progress. This removes an unknown from the central-force radial turning point calculation and helps reduce the Kepler orbit to a radial problem.
There is a historical geometric version of this result. In Book I, Section II, Proposition I of the Principia, Newton proves that motion under a central force toward a fixed centre stays in a plane and sweeps equal areas in equal times, using successive central impulses and equal triangle areas. [ref] In the modern notation above, constant areal velocity is : the old geometric proof and the angular momentum calculation express the same invariant.