The moment of inertia (rotational inertia) is one of the most fundamental quantities in classical mechanics. Just as mass determines how strongly a body resists linear acceleration under a force, the moment of inertia I determines how strongly it resists angular acceleration under a torque. Formally,
τ = I α
where τ is the net torque (N·m), I is the moment of inertia (kg·m²), and α is the angular acceleration (rad/s²). This is Newton’s second law applied to rotation. The moment of inertia appears in rotational kinetic energy, angular momentum, the period of a physical pendulum, and the design of flywheels, gyroscopes, turbines, and vehicle drivetrains.
The defining integral
For a continuous rigid body the moment of inertia about an axis is
I = ∫ r² dm
where r is the perpendicular distance from the mass element dm to the axis. For a discrete collection of point masses this becomes I = Σ mᵢ rᵢ². The integral is evaluated once for each canonical shape and axis combination; the results are the closed-form formulas tabulated below and implemented in this calculator.
Shapes and formulas
| Shape | Axis | Formula |
|---|---|---|
| Solid sphere (mass m, radius r) | Any diameter | I = (2/5) m r² |
| Thin spherical shell | Any diameter | I = (2/3) m r² |
| Solid cylinder (radius r, length L) | Symmetry axis | I = (1/2) m r² |
| Solid cylinder | Transverse mid-length | I = (1/12) m (3r² + L²) |
| Hollow cylinder (outer R, inner r) | Symmetry axis | I = (1/2) m (R² + r²) |
| Thin ring / hoop | Symmetry axis | I = m r² |
| Thin ring / hoop | Diameter | I = (1/2) m r² |
| Thin rod (length L) | Perp. through centre | I = (1/12) m L² |
| Thin rod | Perp. through end | I = (1/3) m L² |
| Rectangular plate (a × b) | x-axis (along a) | I = (1/12) m b² |
| Rectangular plate (a × b) | Normal to plate | I = (1/12) m (a² + b²) |
The parallel axis theorem extends any of these: I = I_cm + m d², where d is the distance from the centre-of-mass axis to the new parallel axis.
Rotational dynamics tab
Once I is computed, the calculator provides three derived quantities for a given angular velocity ω (rad/s):
- Rotational kinetic energy: KE = ½ I ω² (joules)
- Angular momentum: L = I ω (kg·m²/s)
- Torque for α = 1 rad/s²: τ = I · 1 (N·m) — handy for motor sizing
Worked example — flywheel energy storage
A steel flywheel modelled as a solid disk has mass 50 kg and radius 0.4 m. It spins at 3 000 rpm (≈ 314.16 rad/s).
- Moment of inertia: I = (1/2) × 50 × 0.4² = 4 kg·m²
- Rotational KE: ½ × 4 × 314.16² ≈ 197 392 J ≈ 197 kJ
- Angular momentum: 4 × 314.16 ≈ 1 257 kg·m²/s
To mount the disk on bearings located 0.6 m from the shaft centre (e.g. the combined axis of a larger assembly), apply the parallel axis theorem:
I_new = 4 + 50 × 0.6² = 4 + 18 = 22 kg·m²
The bearing axis sees more than five times the rotational resistance. Entering those values in the “Parallel Axis Theorem” preset confirms the result instantly.
Conservation of angular momentum
Where no external torque acts, L = I ω = constant. This is why a spinning figure skater accelerates when pulling their arms inward (reducing I, so ω increases), why a collapsing stellar core forms a rapidly spinning pulsar, and why a gyroscope resists reorientation. The interplay between shape-dependent I and conserved L is at the heart of rigid-body rotational dynamics.
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