Moment of inertia (I) is the rotational analogue of mass: just as mass measures a body's inherent resistance to a change in its state of linear motion (inertia), moment of inertia measures a body's resistance to a change in its state of rotational motion, for rotation about a specific axis. Its SI unit is kg m2, and its dimension is [ML2].
For a single point mass mi at perpendicular distance ri from a fixed axis, the moment of inertia about that axis is I=miri2. For a rigid body made up of many such point masses, the moment of inertia about the axis is the sum over all of them:
I=∑imiri2.
Key contrast with mass. Ordinary mass is (to excellent approximation, ignoring relativistic effects) a fixed, invariant property of a body. Moment of inertia is emphatically not invariant — it depends not only on how much mass a body has, but crucially on exactly how that mass is distributed relative to the chosen axis. The same rigid body has a different moment of inertia for every different axis of rotation one might choose, even axes lying entirely outside the physical body itself.
Computing I for a continuous body. Treating an infinitesimally small mass element dm, at perpendicular distance r from the axis, as a point mass gives dI=(dm)r2; integrating over the whole body gives the moment of inertia of any continuous, uniformly-distributed bulk object:
I=∫dI=∫r2dm.
This integral, carried out with the mass element dm expressed via the object's linear density λ=M/ℓ (for a rod), surface density σ=M/(πR2) (for a disc), or similar, yields the standard results for common shapes:
- Uniform rod (mass M, length ℓ), axis through the center, perpendicular to the rod: I=121Mℓ2; axis through one end: I=31Mℓ2.
- Uniform ring (mass M, radius R), axis through the center, perpendicular to the plane: I=MR2 (every mass element is at the same distance R from the axis, so the integral is trivial). …