This tool lets you explore conservation of angular momentum for a rigid body rotating about a fixed axis. It uses the relation
I₁ ω₁ = I₂ ω₂
When no net external torque acts on a system, its angular momentum stays constant in time. For a rigid body rotating about a fixed axis, the angular momentum L is the product of moment of inertia and angular velocity:
L = I ω
If the mass distribution changes (for example, a figure skater pulling in their arms), the moment of inertia changes and the angular velocity adjusts so that the product Iω remains the same. This gives the conservation equation used by the calculator:
I₁ ω₁ = I₂ ω₂.
This relation follows from the rotational form of Newton’s second law. Torque τ is the rotational analogue of force and equals the rate of change of angular momentum:
τ = .
When the net external torque is zero, dL/dt = 0 and L is constant in time.
The conservation relation can also be written in MathML, which some browsers and screen readers can interpret directly:
Here I₁ and I₂ are the initial and final moments of inertia, and ω₁ and ω₂ are the initial and final angular velocities.
The calculator algebraically rearranges the conservation equation to solve for the unknown quantity. Starting from
I₁ ω₁ = I₂ ω₂,
you can solve for each variable:
ω₂ = (I₁ / I₂) × ω₁
ω₁ = (I₂ / I₁) × ω₂
I₂ = (I₁ ω₁) / ω₂
I₁ = (I₂ ω₂) / ω₁
The calculator automatically detects which field is blank and applies the appropriate rearranged formula.
Consider a simplified model of a figure skater spinning with arms extended. Suppose:
Using conservation of angular momentum,
I₁ ω₁ = I₂ ω₂
Rearrange to solve for ω₂:
ω₂ = (I₁ / I₂) × ω₁
Plug in the numbers:
ω₂ = (4.0 / 2.0) × 2.0 rad/s = 2 × 2.0 rad/s = 4.0 rad/s
So by halving the moment of inertia, the skater doubles their angular speed, while angular momentum L stays constant at
L = I₁ ω₁ = 4.0 × 2.0 = 8.0 kg·m²/s.
The moment of inertia I measures how strongly an object resists changes in its rotational motion about a particular axis. It depends on how mass is distributed relative to that axis:
Because L = I ω must remain constant when no external torque acts, a decrease in I leads to an increase in ω, and vice versa. This trade-off underlies many rotational phenomena, from collapsing gas clouds that spin up as they contract to spinning satellites that use internal mass shifts for control.
When you click Compute, the output gives the missing quantity that makes I₁ ω₁ equal to I₂ ω₂. Interpreting the result:
The same conservation principle appears in many settings. The table below compares a few common scenarios where a simple I₁ ω₁ = I₂ ω₂ model is often reasonable.
| Scenario | What Changes? | When the Simple Model Works | When It Breaks Down |
|---|---|---|---|
| Figure skater spin | Arm position changes, altering I | Short time intervals; friction with ice is small | Long times with significant air drag or strong push from ice |
| Student on a rotating stool | Holding and moving dumbbells in or out | Low external torque from the stool bearings | Large friction torque in the bearing or touching the floor |
| Planetary disk contraction | Gas cloud radius decreases | Idealized, isolated cloud with weak external torques | Strong magnetic torques, outflows, or interactions with other bodies |
| Diver in mid-air | Body configuration changes during a somersault | After leaving the platform and before entering the water | While in contact with the board or water, where large external torques act |
The calculator is intentionally simple. It is based on a one-line conservation law and is best used for introductory physics problems and idealized scenarios. Keep these assumptions and limitations in mind:
If your situation involves large external torques, rapidly changing rotation axes, deformable bodies, or complex multi-body interactions, a more detailed rotational dynamics model is required and this simple conservation calculator will only provide a rough approximation.
Drag the slider arms or tap the canvas to move mass inward and outward, keeping angular velocity inside the target band while the system throws shifting inertia surprises at you.
Balance ω inside the green band.
Tip: Pull mass outward to increase I and slow ω when you overshoot the band.