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Calculators/Momentum
Classical Mechanics

Momentum Calculator

Calculate momentum (p = mv), or solve for mass or velocity. Includes a full collision solver for elastic, inelastic and perfectly inelastic collisions.

Momentum p = mv

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Collision Solver

1D collision — enter masses, velocities and coefficient of restitution (e)

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Momentum equations

Momentum
p = mv
Impulse
J = F·Δt = Δp
Conservation
m₁v₁ + m₂v₂ = const
Elastic collision v₁'
v₁' = (m₁−m₂)v₁/(m₁+m₂) + 2m₂v₂/(m₁+m₂)
Inelastic v_combined
v_f = (m₁v₁+m₂v₂)/(m₁+m₂)
KE from momentum
KE = p²/(2m)

What is momentum?

Momentum is the product of an object's mass and velocity: p = mv. It is a vector quantity — it has both magnitude and direction. The law of conservation of momentum states that the total momentum of a closed system remains constant unless an external force acts on it.

Impulse J = FΔt is the change in momentum caused by a force applied over time. This is why airbags save lives — they increase the time of impact, reducing the force even though the change in momentum (from moving to stationary) is the same. For the full treatment see Momentum and Impulse.

What is the difference between momentum and kinetic energy?
Momentum p = mv is linear in velocity; kinetic energy KE = ½mv² is quadratic. Momentum is always conserved in collisions; kinetic energy is only conserved in perfectly elastic collisions. They measure different aspects of motion.
Why is momentum conserved?
Conservation of momentum follows directly from Newton's third law: if object A exerts a force on object B, then B exerts an equal and opposite force on A. Over any time interval, these forces produce equal and opposite impulses — equal and opposite changes in momentum. The total change is zero.

Momentum and Impulse — The Complete Physics Guide

Momentum is one of the most fundamental conserved quantities in physics. Defined as the product of mass and velocity (p = mv), it represents the "quantity of motion" — a concept that has been central to mechanics since Descartes and Newton debated its nature in the 17th century. The conservation of momentum is one of the most powerful tools in all of physics, applicable to collisions, explosions, rocket propulsion, and the interactions of subatomic particles.

This guide explains momentum and impulse from first principles, derives the conservation law, works through collision examples, and connects momentum to real-world applications from car safety to space travel.

What Is Momentum?

Momentum (p) is a vector quantity — it has both magnitude and direction. The magnitude is p = mv, where m is mass in kg and v is velocity in m/s. The SI unit of momentum is kg·m/s, equivalent to N·s (newton-seconds). Unlike kinetic energy (a scalar), momentum carries directional information: a car moving east has positive momentum, and the same car moving west has negative momentum in our chosen sign convention.

Newton's Second Law in its most general form is F = dp/dt — force equals the rate of change of momentum. For constant mass, this becomes the familiar F = ma. But the general form is more powerful: it handles cases where mass changes (rockets burning fuel) and provided the foundation for Einstein's relativistic mechanics.

The connection between force and momentum gives us the impulse-momentum theorem: the impulse delivered to an object (J = F·Δt, the product of force and the time it acts) equals the change in momentum: J = Δp = mΔv. This reformulation is often more useful than F = ma when we know forces act for specific time intervals rather than over specific distances.

Conservation of Momentum

The conservation of momentum states: in a closed system (no external forces), total momentum is constant. This follows directly from Newton's Third Law: if object A exerts a force on object B, then B exerts an equal and opposite force on A. These forces act for the same time interval, so the impulses are equal and opposite, and the changes in momentum cancel out — total momentum is unchanged.

In mathematical form: m₁v₁ + m₂v₂ = m₁v₁' + m₂v₂' (where primes denote velocities after the event). This equation holds for all collisions and explosions, regardless of how complex the internal forces are. You do not need to know anything about what happens during the collision to apply this law — only the masses and velocities before and after.

Conservation of momentum is one of Noether's theorem's crowning results: it follows directly from the homogeneity of space — the fact that the laws of physics are the same at every location. This deep connection between symmetry and conservation laws is one of the most beautiful results in all of theoretical physics.

Worked Example 1 — Perfectly Inelastic Collision

Problem: A 2,000 kg car travelling at 15 m/s east collides with a stationary 1,000 kg car. They stick together. Find the velocity after collision and the kinetic energy lost.

Momentum before: p = 2000 × 15 + 1000 × 0 = 30,000 kg·m/s east

Velocity after: (2000 + 1000) × v' = 30,000 → v' = 10 m/s east

KE before: ½ × 2000 × 15² = 225,000 J

KE after: ½ × 3000 × 10² = 150,000 J → 75,000 J (33%) lost to heat and deformation

Worked Example 2 — Elastic Collision

Problem: A 3 kg ball moving at 4 m/s collides elastically with a stationary 1 kg ball. Find both final velocities.

For elastic collisions: both momentum AND kinetic energy are conserved. Using the standard elastic collision formulas:

v₁' = (m₁ − m₂)/(m₁ + m₂) × v₁ = (3−1)/(3+1) × 4 = 2/4 × 4 = 2 m/s

v₂' = 2m₁/(m₁ + m₂) × v₁ = 6/4 × 4 = 6 m/s (the lighter ball moves faster!)

Impulse in Engineering and Sport

The impulse-momentum theorem explains many practical engineering choices. The change in momentum of a crash victim is fixed — determined by the car's speed. The question is how to deliver that momentum change safely. A longer collision duration (crumple zones, airbags) means a smaller average force on the occupant for the same total impulse. This is why modern cars are designed to deform progressively rather than remain rigid.

In sports, a cricket or baseball batter "follows through" — extending the time of contact to increase impulse and therefore the change in ball momentum, hitting the ball harder. A martial artist breaks boards by maximising force over a very short contact time — large force, short time, same impulse needed to accelerate the hand through the board.

Rocket propulsion is the ultimate application of momentum conservation. A rocket expels mass (exhaust gas) at high velocity in one direction. By conservation of momentum, the rocket gains equal momentum in the opposite direction. This works in the vacuum of space where there is nothing to push against — unlike a propeller or wheel, rockets need only Newton's Third Law and momentum conservation.

Momentum in Two Dimensions

In two-dimensional collisions, momentum is conserved independently in each direction. This is the principle that allows particle physicists to reconstruct the paths of invisible particles in cloud chambers and bubble chambers — by tracking all visible particle tracks, the momentum of any invisible products can be inferred from the "missing" momentum required to balance the conservation equation.

The 2D elastic collision equations become more complex but the underlying principle is the same: vector momentum before = vector momentum after, with the additional constraint that kinetic energy is conserved. Pool and billiards balls provide everyday examples of 2D elastic collisions, where the geometry of deflection angles is governed entirely by momentum and energy conservation.

Frequently Asked Questions

What is momentum in physics?
Momentum (p = mv) is the product of an object's mass and velocity. It is a vector quantity — it has both magnitude and direction. The SI unit is kg·m/s. Momentum represents the quantity of motion and is conserved in all closed systems (no external forces).
What is the difference between momentum and kinetic energy?
Momentum (p = mv) is a vector, linear in velocity, and always conserved in collisions. Kinetic energy (KE = ½mv²) is a scalar, quadratic in velocity, and only conserved in elastic collisions. They are related by KE = p²/(2m). In inelastic collisions, momentum is conserved but KE is partially converted to heat.
What is impulse?
Impulse (J) is the product of force and the time for which it acts: J = F·Δt. By the impulse-momentum theorem, impulse equals the change in momentum: J = Δp. Impulse is measured in N·s = kg·m/s, the same units as momentum.
Is momentum always conserved?
Momentum is conserved when the net external force on the system is zero. In a collision, external forces (friction, gravity) may act, but during the brief collision time they contribute negligible impulse compared to the collision forces. So for practical purposes, momentum is conserved in all collisions. In an isolated system with no external forces, conservation is exact.
What is the difference between elastic and inelastic collisions?
In an elastic collision, both momentum and kinetic energy are conserved — objects bounce off perfectly, like billiard balls or gas molecule collisions. In an inelastic collision, momentum is conserved but kinetic energy is not — some converts to heat, sound, or deformation. In a perfectly inelastic collision, the objects stick together.

Physics Fundamentals

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