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Angular Momentum (L) kg·m²/s
L (CGS) g·cm²/s
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About

Angular momentum L is the rotational analogue of linear momentum. For a point particle, L = m × v × r × sin(θ). For a rigid body rotating about a fixed axis, L = I × ω, where I is the moment of inertia. Miscalculating I by choosing the wrong geometric model leads to engineering errors in flywheel design, satellite attitude control, and gyroscopic stability analysis. This calculator implements exact formulas for 12 standard rigid-body shapes per classical mechanics references and converts results to SI units (kg⋅m²/s), CGS units (g⋅cm²/s), and reduced Planck constant for quantum-scale work.

Note: all formulas assume uniform mass distribution and rigid-body constraints. Real-world objects with non-uniform density require numerical integration of the inertia tensor. The angle θ in orbital mode is measured between the position vector r and the velocity vector v. At θ = 0° the particle moves radially and L vanishes. Pro tip: for compound shapes, compute each component's I separately and sum via the parallel axis theorem.

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Formulas

Two primary computation modes are supported: orbital angular momentum for point particles and spin angular momentum for rigid bodies rotating about a fixed axis.

Lorbital = m v r sin(θ)

Where m is mass (kg), v is linear velocity (m/s), r is the distance from the rotation axis (m), and θ is the angle between r and v.

Lspin = I ω

Where I is the moment of inertia (kg⋅m²) determined by shape geometry and ω is the angular velocity (rad/s). Angular velocity relates to rotational speed n (RPM) by:

ω = 2πn60

The reduced Planck constant for quantum-scale conversion: = 1.054571817 × 10−34 J⋅s. The CGS conversion factor: 1 kg⋅m²/s = 107 g⋅cm²/s.

Reference Data

ShapeAxisMoment of Inertia INotes
Point massDistance rmr2Orbital only
Solid sphereThrough center25 mr2Uniform density
Hollow sphere (thin shell)Through center23 mr2Shell thickness → 0
Solid cylinder / discCentral axis12 mr2Flywheels, wheels
Hollow cylinder (thin wall)Central axismr2Pipe, hoop
Thick-walled cylinderCentral axis12 m(r12 + r22)r1 inner, r2 outer
Thin rodCenter, perpendicular112 mL2L = rod length
Thin rodEnd, perpendicular13 mL2Pendulum approximation
Rectangular plateCenter, perpendicular112 m(a2 + b2)a, b = side lengths
Solid coneCentral axis310 mr2Base radius r
EllipsoidThrough center, along c15 m(a2 + b2)Semi-axes a, b perpendicular to axis
Torus (ring)Central axism(R2 + 34r2)R = major, r = minor radius
Annular discCentral axis12 m(r12 + r22)Washer, brake disc

Frequently Asked Questions

At θ = 0° or 180°, sin(θ) = 0, which makes the orbital angular momentum L = 0. Physically this means the particle moves purely radially toward or away from the axis, producing no rotational effect. Maximum L occurs at θ = 90°.
The parallel axis theorem states I = Icm + md2, where d is the distance between the center-of-mass axis and the parallel axis. This calculator computes Icm only. If your rotation axis is offset, add the md2 term manually to the displayed I value before computing L.
A thick-walled cylinder has mass distributed between inner radius r1 and outer radius r2. Its moment of inertia is 12m(r12 + r22). Setting r1 = 0 reduces it to a solid cylinder. Setting r1 r2 gives a thin-walled hoop.
This calculator computes classical angular momentum. Quantum spin is an intrinsic property with eigenvalues S = ħs(s + 1), which does not derive from mass or radius. However, the ħ unit output lets you compare classical results against quantum scales.
The calculator handles this automatically. Enter angular velocity in either rad/s or RPM and select the corresponding unit. Internally, RPM is converted via ω = 2π n60. For example, 3000 RPM = 314.16 rad/s.
Yes. All shapes in this calculator assume uniform (homogeneous) density. For objects with variable density ρ(r), you must integrate I = r2 dm numerically. The error from using uniform formulas on non-uniform bodies can exceed 30% for strongly graded materials.