Just as $F=ma$ governs straight-line motion, an exactly parallel law governs rotation. A net torque produces angular acceleration in direct proportion to the torque and inversely to the moment of inertia. This makes rotational dynamics a near-perfect mirror of translational dynamics — every linear quantity has a rotational twin.
The rotational equation of motion is:
- $\tau=I\alpha$, where $\alpha$ is the angular acceleration ($\text{rad/s}^2$) — the rotational analogue of $F=ma$.
- The work done by a torque through an angle $\theta$ is $W=\tau\theta$, and the power delivered is $P=\tau\omega$.
- Rotational kinetic energy: a body rotating with angular speed $\omega$ stores energy $KE_{rot}=\frac{1}{2}I\omega^2$, the analogue of $\frac{1}{2}mv^2$.
- Work–energy theorem for rotation: $W_{net}=\Delta KE_{rot}=\frac{1}{2}I\omega_2^2-\frac{1}{2}I\omega_1^2$.
Rolling without slipping combines translation of the centre of mass with rotation about it. The key condition is that the contact point is instantaneously at rest, which links the two motions:
- $v=\omega R$ (velocity of the centre) and $a=\alpha R$ (acceleration), where $R$ is the radius.
- The total kinetic energy is the sum of translational and rotational parts: $KE=\frac{1}{2}mv^2+\frac{1}{2}I\omega^2$.
- Using $I=mk^2$ and $v=\omega R$, this becomes $KE=\frac{1}{2}mv^2\left(1+\frac{k^2}{R^2}\right)$.
Rolling down an incline. When a body rolls (without slipping) down a slope of height $h$, the lost potential energy $mgh$ becomes shared between translational and rotational KE. Solving energy conservation gives the speed at the bottom and the acceleration along the incline:
- $v=\sqrt{\dfrac{2gh}{1+\frac{k^2}{R^2}}}$ and $a=\dfrac{g\sin\theta}{1+\frac{k^2}{R^2}}$.
- Because $\frac{k^2}{R^2}$ is smallest for a sphere ($\tfrac{2}{5}$), larger for a disc ($\tfrac{1}{2}$), and largest for a ring ($1$), a solid sphere reaches the bottom first, then the disc, then the ring — regardless of mass or radius.