Interactive module Rigid-body dynamics

Angular Momentum

Why does a satellite spin faster as its booms fold in, a bullet set a heavy door swinging, and a gyroscope float sideways instead of falling? Angular momentum answers all three. This module, written for second-year mechanical and aerospace engineering students, starts with a single particle and builds up to the 3D motion of rigid bodies, gyroscopes and tops, in eight lessons with live simulations and questions that check your work.

  • 8 lessons
  • about 4¾ h of lessons
  • Works offline

Show

A gyroscope supported at one end of its axle, simulated with the full equations of motion. Gravity's moment \(\colM{\Mvec_O}\) about the support is horizontal, so the angular momentum \(\colH{\Hvec_O}\), along the spinning axle, swings sideways toward it instead of falling: \(\Mvec_O = \dot{\Hvec}_O\). The whole module leads up to explaining this picture.

Learning outcomes

By the end of the module you can:

  • Compute the angular momentum of a particle, \(\Hvec_O = \rvec \times m\vvec\), in 2D and 3D. (Lesson 1)
  • Apply \(\sum\Mvec_O = \dot{\Hvec}_O\), angular impulse and conservation of angular momentum to particles and central-force motion. (Lesson 2)
  • Use \(\Hvec_O = \rvec_G \times m\vvec_G + \Hvec_G\) and the moment equations for systems of particles. (Lesson 3)
  • Find the angular momentum of a rigid body in plane motion about any point, and connect it to \(\sum M_G = I_G\alpha\). (Lesson 4)
  • Solve impulse, impact and coupling problems for rigid bodies, including the center of percussion. (Lesson 5)
  • Compute \(\Hvec = \Imat\wvec\) and the kinetic energy of a body in 3D, and apply Euler's equations. (Lessons 6–7)
  • Analyze gyroscopic moments, steady precession of tops and gyroscopes, and torque-free motion. (Lesson 8)

How to use this module

Before you start: you should be comfortable with vector cross products, Newton's second law and impulse–momentum for particles, plane rigid-body kinematics, and moments of inertia (the Mass Moments of Inertia module covers the inertia tensor used in Lessons 6–8).

Work through the lessons in order. The times allow for working the examples on paper and doing the checks. A suggested plan in four sittings:

  1. Lessons 1–265 min

    Angular momentum of a particle, the moment equation, angular impulse and conservation.

  2. Lessons 3–465 min

    Systems of particles and rigid bodies in plane motion.

  3. Lessons 5–675 min

    Impulse, impact and couplings of rigid bodies; angular momentum in 3D.

  4. Lessons 7–8, Practice Lab and Self-Check Quiz140 min

    Euler's equations and gyroscopic motion, about 30 min of practice, then the 35-minute quiz.

About 5¾ h in total:280 min of lessons, 30 min of practice, 35 min for the quiz

Get the most out of it

Lessons

Each lesson has interactive figures, worked examples and questions with instant feedback.

Practice, tools and reference

Use these alongside the lessons, or on their own when you revise.

Requirements

Any modern browser. Works offline.

  • A current version of Chrome, Edge, Firefox or Safari, with JavaScript on. A laptop or desktop screen works best; the pages also fit tablets and phones.
  • The 3D figures need WebGL, which every current browser has. If it is turned off, the figures show a short message and the rest of the page still works.
  • No internet connection, installation or account. Everything is inside this folder.
  • Your progress is saved in this browser on this device. Private or incognito windows do not keep it.

Something not working? Read README.txt in the module folder for how to open the module and fix common problems.