Physics

Angular Momentum

Conservation of Angular Momentum

Physics
NEET UG
Version 1Updated 22 Mar 2026

The principle of conservation of angular momentum states that if the net external torque acting on a system is zero, then the total angular momentum of the system remains constant. This fundamental principle is a direct consequence of Newton's second law for rotational motion, which posits that the rate of change of angular momentum of a system is equal to the net external torque acting on it. Mat…

Quick Summary

The Conservation of Angular Momentum is a fundamental principle stating that the total angular momentum of a system remains constant if the net external torque acting on it is zero. Angular momentum (L\vec{L}) is the rotational equivalent of linear momentum, defined as L=Iω\vec{L} = I\vec{\omega} for a rigid body, where II is the moment of inertia and ω\vec{\omega} is the angular velocity.

The principle arises directly from Newton's second law for rotation, τext=dLdt\vec{\tau}_{ext} = \frac{d\vec{L}}{dt}. If τext=0\vec{\tau}_{ext} = 0, then L\vec{L} is constant. This means that if the moment of inertia (II) of a system changes (e.

g., by redistributing mass), its angular velocity (ω\omega) must change inversely to maintain a constant IωI\omega. This principle explains phenomena like ice skaters spinning faster when they pull their arms in, divers tucking for somersaults, and the constant areal velocity of planets in orbit.

It's crucial to remember that angular momentum is a vector quantity, and its conservation implies both constant magnitude and direction. Rotational kinetic energy is generally not conserved when angular momentum is conserved if II changes.

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Key Concepts

Angular Momentum (L = Iω\omega)

Angular momentum is a measure of an object's rotational motion. For a rigid body rotating about a fixed axis,…

Moment of Inertia (I)

Moment of inertia is a critical concept in rotational dynamics, analogous to mass in linear motion. It…

External Torque (τext\vec{\tau}_{ext})

External torque is the rotational equivalent of an external force. It is a twisting action that tends to…

  • Condition:Net external torque τext=0\vec{\tau}_{ext} = 0.
  • Principle:Total angular momentum L\vec{L} of the system remains constant.
  • Formula (rigid body):L=Iω=constantL = I\omega = \text{constant}.
  • Conservation Equation:I1ω1=I2ω2I_1\omega_1 = I_2\omega_2.
  • Angular Momentum (particle):L=r×p\vec{L} = \vec{r} \times \vec{p}.
  • Torque:τ=r×F\vec{\tau} = \vec{r} \times \vec{F}.
  • Rotational Kinetic Energy:Krot=12Iω2=L22IK_{rot} = \frac{1}{2}I\omega^2 = \frac{L^2}{2I}. (NOT conserved if II changes, even if LL is conserved).
  • Key Examples:Ice skater, diver, planetary motion, rotating platforms, rotational collisions.

Let It Often Conserve: L (Angular Momentum) is conserved if Internal forces only act, or Outside torques Cancel out.

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