Angular Momentum Calculator
Calculate the angular momentum of an object using moment of inertia
Input Parameters
For Angular Momentum (L)
For Linear Momentum (p)
This calculator computes angular momentum, the rotational equivalent of linear momentum. [1, 2, 4] It is a conserved quantity, meaning it remains constant unless an external torque acts on the system. [2, 3]
- Angular Momentum (L): The product of an object's moment of inertia and its angular velocity. [1]
- Linear Momentum (p): The product of an object's mass and its linear velocity. [1]
L = I × ω
p = m × v
Enter parameters and click Calculate
About Angular Momentum Calculator
The Universe's Spin: A Master Guide to Our Angular Momentum Calculator
Watch an ice skater pull in their arms and spin faster. Observe a planet speed up as it gets closer to its star. See how a gyroscope resists being tilted. These seemingly unrelated phenomena are all governed by one of the most profound and fundamental conservation laws in the universe: the **Conservation of Angular Momentum**.
Just as linear momentum describes an object's "quantity of motion" in a straight line, **angular momentum** (`L`) describes its "quantity of rotational motion." It is the rotational equivalent of linear momentum and is a measure of how much effort is required to stop an object from spinning. More importantly, in a closed system, it is a quantity that never changes.
Welcome to the definitive guide to this cornerstone of physics. Our Angular Momentum Calculator is a tool designed to help you quantify this crucial value for both single particles and rotating rigid bodies. This comprehensive article will not only guide you through the calculator's use but will also take you on a deep dive into the physics, revealing the elegant principles that explain everything from the stability of a bicycle to the formation of galaxies.
What is Angular Momentum? Inertia in Rotation
Angular momentum is a measure of an object's rotational inertia. It depends not just on how fast an object is spinning, but also on its mass and how that mass is distributed relative to the axis of rotation.
Like its linear counterpart, angular momentum is a **vector quantity**. It has both a magnitude (how much rotational motion) and a direction. The direction is determined by the **right-hand rule**: if you curl the fingers of your right hand in the direction of the object's rotation, your thumb points in the direction of the angular momentum vector, which lies along the axis of rotation.
Our calculator can compute angular momentum for two primary scenarios.
Scenario 1: Angular Momentum of a Single Particle
Consider a single particle of mass `m` moving with a linear velocity `v` at a distance `r` from a central point. This could be a planet orbiting the sun or a ball being swung on a string. Its angular momentum `L` is defined as the cross product of its position vector `r` and its linear momentum vector `p` (`p = mv`).
The magnitude of the angular momentum for a particle in circular motion (or at the point of closest approach) is given by a simpler formula:
- L is the angular momentum, measured in **kilogram-meters squared per second (kg·m²/s)**.
- r is the **radius** of the circular path or the distance from the pivot point, in meters (m).
- m is the **mass** of the particle in kilograms (kg).
- v is the **linear (tangential) velocity** of the particle in meters per second (m/s).
Scenario 2: Angular Momentum of a Rotating Rigid Body
For a solid, extended object that is rotating (like a spinning wheel, a planet rotating on its axis, or a spinning top), we use a different but analogous formula. We need to know how the object's mass is distributed.
- L is the angular momentum (kg·m²/s).
- I is the **Moment of Inertia** of the object. This is the rotational equivalent of mass. It measures an object's resistance to being spun up or slowed down. Its value depends on the object's mass and, critically, how that mass is shaped and distributed around the axis of rotation. It is measured in **kg·m²**.
- ω (omega) is the angular velocity of the object, measured in radians per second (rad/s).
Notice the beautiful parallel between the linear and rotational formulas:
Linear Momentum
p = m * v
Angular Momentum
L = I * ω
How to Use the Angular Momentum Calculator
Step 1: Select the Scenario
Choose whether you are calculating for a **Single Particle** in orbit or a **Rotating Rigid Body**. This will present the correct set of inputs.
Step 2: Enter the Variables
For a Single Particle:
- Enter the **Mass (m)** in kg.
- Enter the **Velocity (v)** in m/s.
- Enter the **Radius (r)** in meters.
For a Rotating Rigid Body:
- Enter the **Moment of Inertia (I)** in kg·m². (You may need to calculate this first based on the object's shape).
- Enter the **Angular Velocity (ω)** in rad/s. (Our calculator can help convert from common units like RPM).
Step 3: View the Result
The calculator will instantly compute the angular momentum `L` in its standard SI unit of kg·m²/s.
The Law of Conservation of Angular Momentum
This is where the concept becomes truly powerful. The law states that if no **external torque** acts on a rotating system, its total angular momentum (`L`) will remain constant. A torque is a rotational force—a twist or a turn.
This means `I_initial * ω_initial = I_final * ω_final`. This single equation explains a vast range of phenomena.
Example: The Spinning Ice Skater
An ice skater begins a spin with her arms outstretched. She then pulls her arms in tight to her body.
- • Initial State (Arms Out): Her mass is distributed far from her axis of rotation. This gives her a **large Moment of Inertia (I_initial)**. She spins with a certain angular velocity (ω_initial).
- • Final State (Arms In): By pulling her arms in, she brings her mass closer to the axis of rotation. This **decreases her Moment of Inertia (I_final)**.
- • Conservation in Action: Since no external torque is acting on her (we can ignore the tiny friction from the ice), her angular momentum `L` must stay the same. Because `L = I * ω` must be constant, and `I` has decreased, her angular velocity `ω` **must increase** to compensate. She spins dramatically faster.
Real-World Examples and Importance
Planetary Orbits
Planets move in elliptical orbits. As a planet gets closer to its star (`r` decreases), its angular momentum (`L=rmv`) must be conserved. To compensate for the smaller radius, its velocity (`v`) must increase. This is why planets move fastest at perihelion (closest approach) and slowest at aphelion (farthest point).
Gyroscopic Stability
A spinning top, a gyroscope, or even a rifle bullet is stable because of its angular momentum. The spinning gives it a large `L` vector. To change the direction of this vector (i.e., to make the object wobble or tumble), an external torque must be applied. The object's angular momentum gives it "gyroscopic inertia" that resists this change in orientation, keeping it stable.
Diving and Gymnastics
A diver leaves the board with a certain amount of angular momentum. By tucking into a tight ball (`I` decreases), they can increase their rotational speed (`ω` increases) to perform multiple somersaults. By extending their body before hitting the water (`I` increases), they slow their rotation (`ω` decreases) for a clean entry.
Galaxy Formation
A vast, slow-rotating cloud of gas and dust in space has an enormous amount of angular momentum due to its sheer size. As gravity pulls this cloud together to form a star and planets, its overall radius `r` decreases dramatically. To conserve angular momentum, its rotational speed `ω` must increase immensely, leading to the formation of a spinning protostellar disk from which planets are born.
Frequently Asked Questions (FAQ)
Q: How do I find the Moment of Inertia (I)?
The Moment of Inertia depends on the shape of the object. For simple shapes, there are standard formulas (e.g., for a solid sphere, `I = (2/5)mr²`; for a solid disk, `I = ½mr²`). For complex shapes like a car or a human body, it is usually determined experimentally or through computer-aided design (CAD) software.
Q: What is a "torque"?
Torque (`τ`) is the rotational equivalent of force. Just as a net force causes a change in linear momentum, a net torque causes a change in angular momentum (`τ = ΔL / Δt`). If you want to make something start spinning, stop spinning, or change its axis of spin, you must apply a torque.
A Pillar of Modern Physics
The conservation of angular momentum is a principle that holds true from the quantum level of electron spin to the cosmic scale of galactic rotation. It is a concept of breathtaking scope and elegance. Understanding it is essential for anyone serious about physics, astronomy, or engineering.
Use our calculator to quantify the "quantity of rotation" in various systems. Explore how changing mass distribution affects angular velocity. Calculate the immense angular momentum of our own planet and gain a new appreciation for the universal law that keeps our world spinning steadily on its axis.
Frequently Asked Questions
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