Moment of Inertia by Integration and the Parallel-Axis Theorem
Moment of inertia is an integral of distance squared over the mass distribution, so it depends on the axis as well as the body. The parallel-axis theorem moves a known result to any parallel axis without redoing the integral.
What a learner can do afterwards
- Sets up and evaluates the integral for a rod, a disc or a hoop about a stated axis
- Applies the parallel-axis theorem and says why the moment of inertia is smallest about the centre of mass
- Explains why the same body has different moments of inertia about different axes
1 · Read
Moment of inertia is built piece by piece: chop the body into tiny bits, multiply each bit by its squared distance from the axis, and integrate. Far flung mass counts far more, because distance enters squared. That is why the same body has different moments about different axes: move the same mass outward and I grows, so spin changes meet more resistance.
Symmetry picks the result. A rod gives one twelfth M L squared about its centre, a hoop gives M R squared with all mass at the rim, and a disc lands in between. So for equal mass and radius, the hoop beats the disc. Just as linear kinetic energy is half m v squared, rotational kinetic energy is half I omega squared: with I equal to 3 and omega 2, the energy is 6.
The parallel-axis theorem moves a known result to any parallel axis without redoing the integral: add M times the squared shift distance to the centre of mass value. Shifting the axis always raises I, which is why I is smallest about the centre of mass. For a rod of mass 2 and length 6, the centre value is 6, and shifting 3 to the end adds 2 times 3 squared, giving 24.
Square the distance, integrate over the mass, shift axes with M d squared, and spin energy follows half I omega squared.
2 · Watch
Take it off screen
Where it sits
Where this leads
Jobs that lean on this skill. Follow one to see everything it is built on.
8 questions wait behind this lesson, each with its answer explained. Every answer feeds the sky: stars light as they are learned, and dim when it is time to come back.