Advanced Momentum Calculator

Momentum Configuration

Linear Momentum
Collisions
Angular Momentum
Impulse & Change
Relativistic
Presets
Saved Setups

Object 1

Object 2

0 (Perfectly Inelastic) 0.5 1 (Perfectly Elastic)

When dealing with objects moving at speeds approaching the speed of light, classical momentum calculations are inadequate and relativistic effects must be considered.

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Relativistic Momentum Formula:
p = γmv = mv / √(1 - v²/c²)

Where:

  • p = relativistic momentum
  • m = rest mass
  • v = velocity
  • γ (gamma) = Lorentz factor = 1 / √(1 - v²/c²)
  • c = speed of light (299,792,458 m/s)

Common Momentum Presets

Car Collision

Two vehicles of different masses

Billiard Ball Collision

Elastic collision between equal masses

Ballistic Pendulum

Projectile embeds in swing (inelastic)

Rocket Propulsion

Conservation of momentum (variable mass)

Spinning Ice Skater

Conservation of angular momentum

Pendulum Wave

Multiple pendulums with related periods

Electron Motion

Relativistic effects at high speeds

Recoil Problem

Gun firing bullet (momentum conservation)

Physics Education Examples

Conservation Law Demo

Before and after collision analysis

Impulse Example

Force-time graph analysis

Collision Types

Compare elastic vs. inelastic

Space Physics

Momentum in zero-gravity environment

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Your Saved Setups

Standard Collision
Angular Demo

Momentum Analysis Results

Total Momentum (x)

-1.0
kg·m/s

Total Momentum (y)

0.0
kg·m/s

Momentum Magnitude

1.0
kg·m/s

Direction Angle

180.0
degrees
Visualization
Detailed Analysis
Step-by-Step Calculations
Applications
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Individual Object Analysis

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Object Mass (kg) Velocity (m/s) Momentum (kg·m/s) Kinetic Energy (J)
Object 1 1.0 5.0 5.0 12.5
Object 2 2.0 -3.0 -6.0 9.0

Conservation Analysis

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Property Before After Change Conservation
Total Momentum (x) -1.0 kg·m/s -1.0 kg·m/s 0.0 kg·m/s
Total Momentum (y) 0.0 kg·m/s 0.0 kg·m/s 0.0 kg·m/s
Total Kinetic Energy 21.5 J 21.5 J 0.0 J

Vector Components

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Object Momentum (x) kg·m/s Momentum (y) kg·m/s Magnitude kg·m/s Direction (°)
Object 1 5.0 0.0 5.0 0.0
Object 2 -6.0 0.0 6.0 180.0
System Total -1.0 0.0 1.0 180.0
1. Calculating Individual Momentum Values

For each object, momentum is calculated using the formula:

p = mv

Object 1:

  • Mass (m₁) = 1.0 kg
  • Velocity (v₁ˣ) = 5.0 m/s
  • Velocity (v₁ʸ) = 0.0 m/s
  • Momentum (p₁ˣ) = m₁ × v₁ˣ = 1.0 kg × 5.0 m/s = 5.0 kg·m/s
  • Momentum (p₁ʸ) = m₁ × v₁ʸ = 1.0 kg × 0.0 m/s = 0.0 kg·m/s

Object 2:

  • Mass (m₂) = 2.0 kg
  • Velocity (v₂ˣ) = -3.0 m/s
  • Velocity (v₂ʸ) = 0.0 m/s
  • Momentum (p₂ˣ) = m₂ × v₂ˣ = 2.0 kg × (-3.0 m/s) = -6.0 kg·m/s
  • Momentum (p₂ʸ) = m₂ × v₂ʸ = 2.0 kg × 0.0 m/s = 0.0 kg·m/s
2. Computing System Total Momentum

The total momentum of the system is the vector sum of all individual momenta:

ptotal = p₁ + p₂ + ... + pₙ

X-Component:

  • ptotal,x = p₁ˣ + p₂ˣ
  • ptotal,x = 5.0 kg·m/s + (-6.0 kg·m/s)
  • ptotal,x = -1.0 kg·m/s

Y-Component:

  • ptotal,y = p₁ʸ + p₂ʸ
  • ptotal,y = 0.0 kg·m/s + 0.0 kg·m/s
  • ptotal,y = 0.0 kg·m/s

Momentum Magnitude:

  • |ptotal| = √(ptotal,x² + ptotal,y²)
  • |ptotal| = √((-1.0 kg·m/s)² + (0.0 kg·m/s)²)
  • |ptotal| = √(1.0 (kg·m/s)²)
  • |ptotal| = 1.0 kg·m/s

Direction Angle:

  • θ = tan⁻¹(ptotal,y / ptotal,x)
  • θ = tan⁻¹(0.0 / -1.0)
  • θ = 180.0° (adjusting for the negative x-component)
3. Kinetic Energy Analysis

Kinetic energy for each object is calculated using:

KE = ½mv²

Object 1:

  • KE₁ = ½ × m₁ × v₁²
  • KE₁ = ½ × 1.0 kg × (5.0 m/s)²
  • KE₁ = ½ × 1.0 kg × 25.0 (m/s)²
  • KE₁ = 12.5 J

Object 2:

  • KE₂ = ½ × m₂ × v₂²
  • KE₂ = ½ × 2.0 kg × (-3.0 m/s)²
  • KE₂ = ½ × 2.0 kg × 9.0 (m/s)²
  • KE₂ = 9.0 J

Total Kinetic Energy:

  • KEtotal = KE₁ + KE₂
  • KEtotal = 12.5 J + 9.0 J
  • KEtotal = 21.5 J

Real-World Applications

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  • Vehicle Safety: Momentum analysis is fundamental to crash test design and safety systems. A vehicle's momentum is redirected and absorbed during collisions to minimize impact force on passengers.
  • Sports Physics: Momentum transfer is critical in sports like billiards, bowling, golf, and baseball, where the momentum of one object (club, ball, bat) is transferred to another.
  • Rocketry and Space Travel: Rockets operate on the principle of conservation of momentum, expelling mass (exhaust) in one direction to gain momentum in the opposite direction.
  • Ballistics: Momentum calculations are essential for understanding projectile motion, recoil, and impact forces.
  • Engineering Design: Momentum considerations affect the design of hydraulic systems, turbines, and mechanical components that involve flowing fluids or moving parts.

Connection to Other Physics Concepts

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  • Newton's Laws: Momentum is directly related to Newton's second law (F = dp/dt) and third law (equal and opposite reactions).
  • Energy Conservation: While momentum is always conserved in closed systems, kinetic energy is only conserved in elastic collisions.
  • Relativistic Effects: At speeds approaching the speed of light, classical momentum must be replaced with relativistic momentum calculations.
  • Quantum Mechanics: In quantum physics, particles have wave-like properties, and momentum is related to wavelength through de Broglie's equation (p = h/λ).
  • Fluid Dynamics: Momentum principles apply to flowing fluids and are essential in understanding pressure, drag, and lift forces.

Practical Examples for Your Calculated Values

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Based on your calculated total momentum of 1.0 kg·m/s:

  • This is roughly equivalent to the momentum of a 1 kg textbook moving at walking speed (1 m/s).
  • To stop this momentum in 0.1 seconds would require a force of 10 Newtons, about the weight of a 1 kg mass on Earth.
  • In an elastic collision with a stationary object of equal mass, this momentum would cause the stationary object to move at 1 m/s.
Momentum Theory
Key Formulas
Worked Examples
Physics Glossary

Understanding Momentum in Physics

Momentum is a fundamental concept in physics that describes the quantity of motion an object possesses. It is a vector quantity with both magnitude and direction, defined as the product of an object's mass and velocity.

Key principles of momentum include:

  • Conservation of Momentum: In a closed system (no external forces), the total momentum remains constant. This is one of the most fundamental conservation laws in physics.
  • Impulse-Momentum Theorem: The change in momentum of an object equals the impulse applied to it (the product of force and time).
  • Collisions: Momentum analysis is particularly useful for understanding collisions between objects, which can be classified as elastic (kinetic energy conserved), inelastic (some kinetic energy lost), or perfectly inelastic (objects stick together).

Types of Momentum

  • Linear Momentum: The product of mass and linear velocity (p = mv).
  • Angular Momentum: Describes rotational motion, calculated as the product of moment of inertia and angular velocity (L = Iω).
  • Relativistic Momentum: For objects moving at speeds approaching the speed of light, classical momentum formulas must be modified to account for relativistic effects.

Essential Momentum Formulas

Linear Momentum
p = mv

Where:

  • p = momentum (kg·m/s in SI units)
  • m = mass (kg)
  • v = velocity (m/s)
Impulse-Momentum Theorem
J = Δp = F·Δt

Where:

  • J = impulse (N·s)
  • Δp = change in momentum (kg·m/s)
  • F = force (N)
  • Δt = time interval (s)
Conservation of Momentum
pinitial = pfinal
m₁v₁ + m₂v₂ = m₁v₁' + m₂v₂'

Where:

  • m₁, m₂ = masses of objects
  • v₁, v₂ = initial velocities
  • v₁', v₂' = final velocities
Elastic Collision (1D)
v₁' = ((m₁-m₂)/(m₁+m₂))v₁ + ((2m₂)/(m₁+m₂))v₂
v₂' = ((2m₁)/(m₁+m₂))v₁ + ((m₂-m₁)/(m₁+m₂))v₂
Perfectly Inelastic Collision
v' = (m₁v₁ + m₂v₂)/(m₁ + m₂)

Where v' is the common final velocity

Angular Momentum
L = Iω
L = r × p

Where:

  • L = angular momentum (kg·m²/s)
  • I = moment of inertia (kg·m²)
  • ω = angular velocity (rad/s)
  • r = position vector (m)
  • p = linear momentum (kg·m/s)
  • × = cross product
Relativistic Momentum
p = γmv = mv/√(1-v²/c²)

Where:

  • γ (gamma) = Lorentz factor = 1/√(1-v²/c²)
  • c = speed of light (299,792,458 m/s)

Worked Momentum Problems

Example 1: Elastic Collision

Problem: A 2 kg object moving at 3 m/s collides elastically with a stationary 1 kg object. Find the final velocities of both objects.

Solution:

  1. Initial momentum: pi = m₁v₁ + m₂v₂ = (2 kg)(3 m/s) + (1 kg)(0 m/s) = 6 kg·m/s
  2. For elastic collisions in 1D, use the formulas:
    • v₁' = ((m₁-m₂)/(m₁+m₂))v₁ + ((2m₂)/(m₁+m₂))v₂
    • v₂' = ((2m₁)/(m₁+m₂))v₁ + ((m₂-m₁)/(m₁+m₂))v₂
  3. Substituting our values:
    • v₁' = ((2-1)/(2+1))(3) + ((2×1)/(2+1))(0) = (1/3)(3) = 1 m/s
    • v₂' = ((2×2)/(2+1))(3) + ((1-2)/(2+1))(0) = (4/3)(3) = 4 m/s
  4. Verification:
    • Final momentum: pf = m₁v₁' + m₂v₂' = (2 kg)(1 m/s) + (1 kg)(4 m/s) = 2 + 4 = 6 kg·m/s
    • Initial KE: KEi = ½m₁v₁² = ½(2)(3)² = 9 J
    • Final KE: KEf = ½m₁v₁'² + ½m₂v₂'² = ½(2)(1)² + ½(1)(4)² = 1 + 8 = 9 J

Both momentum and kinetic energy are conserved, confirming an elastic collision.

Example 2: Impulse Problem

Problem: A 150g baseball traveling at 40 m/s is hit by a bat, changing its direction. If the ball leaves with a velocity of 60 m/s in the opposite direction, what impulse was delivered by the bat?

Solution:

  1. Convert to kg: m = 0.150 kg
  2. Initial momentum: pi = mvi = (0.150 kg)(40 m/s) = 6 kg·m/s
  3. Final momentum: pf = mvf = (0.150 kg)(-60 m/s) = -9 kg·m/s (negative because direction is reversed)
  4. Impulse = change in momentum: J = Δp = pf - pi = -9 - 6 = -15 kg·m/s (or 15 kg·m/s in the opposite direction)

The bat delivered an impulse of 15 N·s in the direction opposite to the ball's initial motion.

Example 3: Angular Momentum

Problem: An ice skater with moment of inertia 5 kg·m² is spinning at 2 rad/s with arms extended. When she pulls her arms in, her moment of inertia reduces to 2 kg·m². What is her new angular velocity?

Solution:

  1. Initial angular momentum: Li = Iiωi = (5 kg·m²)(2 rad/s) = 10 kg·m²/s
  2. By conservation of angular momentum (no external torque): Li = Lf
  3. Lf = Ifωf = 10 kg·m²/s
  4. Solving for final angular velocity: ωf = Lf/If = 10 kg·m²/s / 2 kg·m² = 5 rad/s

Her angular velocity increases to 5 rad/s, demonstrating how decreasing moment of inertia results in faster rotation.

Physics Glossary: Momentum Terms

Momentum (p)
The product of an object's mass and velocity, a vector quantity measured in kg·m/s (SI units).
Impulse (J)
The product of force and time interval over which the force acts, equal to the change in momentum.
Elastic Collision
A collision in which both momentum and kinetic energy are conserved.
Inelastic Collision
A collision in which momentum is conserved, but kinetic energy is not fully conserved.
Perfectly Inelastic Collision
A collision in which the objects stick together afterward, moving with a common velocity.
Coefficient of Restitution (e)
A measure of the elasticity of a collision, ranging from 0 (perfectly inelastic) to 1 (perfectly elastic).
Angular Momentum (L)
The rotational equivalent of linear momentum, calculated as the product of moment of inertia and angular velocity.
Moment of Inertia (I)
A measure of an object's resistance to changes in its rotational motion, analogous to mass in linear motion.
Center of Mass
The point at which the weighted relative position of the distributed mass sums to zero.
Relativistic Momentum
The momentum calculation modified to account for special relativity at speeds approaching the speed of light.
Ballistic Pendulum
A device that captures a projectile and uses the principle of momentum conservation to determine the projectile's initial velocity.
Conservation Law
A principle stating that a particular property of an isolated system remains constant despite changes within the system.
Lorentz Factor (γ)
A factor that appears in relativistic equations, defined as 1/√(1-v²/c²).