Energy of rotation
A spinning flywheel is clearly doing something energetic even though its center goes nowhere. Its energy is rotational kinetic energy, and it is the perfect echo of \tfrac12 mv^2 with I replacing m and \omega replacing v.
Rotational kinetic energy uses moment of inertia and angular velocity where linear KE uses mass and speed.
An object that both moves and spins — a rolling ball — carries both kinds at once. Its total kinetic energy is simply the sum:
The kinetic energy of a rolling body splits into translation of its center of mass plus rotation about it.
Rolling without slipping
A wheel that grips the road rolls without slipping: it does not skid, so the point touching the ground is, for that instant, perfectly still. This locks the spin to the travel — one rotation moves the wheel forward exactly one circumference.
The rolling-without-slipping condition ties the center's speed to the spin — the same v = rω, now for the whole wheel's advance.
Angular momentum: rotation's momentum
Just as linear momentum p = mv measures 'how hard it is to stop' a moving object, angular momentum L measures how hard it is to stop a spinning one. For a rigid body it is moment of inertia times angular velocity; for a single particle it is L = mvr about the axis.
Angular momentum is the rotational partner of linear momentum, with I and ω in place of m and v.
Angular momentum is a vector, and like \vec\omega it points along the axis by the right-hand rule. That vector nature is why spinning things are directionally stubborn — a moving bicycle, a thrown football, a rifle bullet all stay pointed where their spin axis points.
Conservation of angular momentum
Here is the payoff. If no external torque acts on a system, its total angular momentum cannot change — this is the conservation of angular momentum, as fundamental as conservation of energy or momentum. So if the object reshapes itself to a smaller I, its \omega must rise to keep L = I\omega fixed.
With no external torque, shrinking I forces ω up — the physics of the spinning skater.
A figure skater spins slowly with arms out, then pulls them in: her I drops, so her \omega shoots up and she blurs. A collapsing star doing the same becomes a pulsar spinning hundreds of times a second. A cat rights itself in mid-air by twisting one part against another with total L staying zero.
Why it holds: torque changes angular momentum
The deep reason is the most general form of Newton's second law for rotation: torque is the rate of change of angular momentum, mirroring F = dp/dt. If the net external torque is zero, L has zero rate of change — it is conserved. Every example above is this one equation in disguise.
The most general rotational Newton's second law: torque is the rate of change of angular momentum.
This vector equation also explains gyroscopes: a torque that is sideways to \vec L does not slow the spin but swings its direction, making the axis sweep in a slow cone — precession. It is why a spinning top does not fall over and how a gyrocompass finds north.