Newtonian mechanics
Moment of inertia and rotational motion
Moment of inertia I=∫r²dm measures mass distribution about an axis and is the rotational analogue of inertia.
Two equal-mass objects resist angular acceleration differently when one has more mass farther from the axis. Moment of inertia depends on mass and its distance from the axis.
Definition: Moment of inertia
is the perpendicular distance of each mass element from the axis; is in kg·m². The relation applies to a rigid body about a fixed axis. General 3D rotation about changing axes requires the inertia tensor.
Standard results
| Body and axis | Moment of inertia |
|---|---|
| Thin hoop, symmetry axis | |
| Solid disk, symmetry axis | |
| Thin rod length , central axis |
These formulas assume uniform bodies and the stated axes. The parallel-axis theorem is for parallel axes offset by .
Example: A disk under torque
A solid disk has kg, m, and net torque N·m. Find its angular acceleration.
Solution
kg·m²; rad/s².
Quick check
For a thin hoop, every mass element lies a distance from the axis, so . In a uniform solid disk, mass lies closer to the axis on average, and integrating over concentric rings gives . Under a constant torque about a fixed axis, angular acceleration is ; moving mass farther from the axis therefore makes rotation harder to accelerate even at unchanged total mass.
Moment of inertia depends on the selected axis because perpendicular distances change when the axis changes. The parallel-axis theorem transfers a result from the center-of-mass axis to a parallel one: . For example, a thin rod of length about one end has , larger than about its center. State both the body and axis before using a formula table.
The unit kg·m² reflects both mass and squared distance from the axis; doubling every distance makes four times larger. Always state the axis alongside its numerical value.
Which has greater I: a hoop or disk with the same M and R about the symmetry axis?
What rotational equation applies to a rigid body about a fixed axis?
References
- John R. Taylor (2005). Classical Mechanics