Mechanics · Simulation
20 April 2026 · on the concept map
Newton's Laws of Motion — Interactive Simulator
Newton's three laws of motion are the foundation of classical mechanics. Published in 1687 in the Principia Mathematica, they describe how objects behave when forces act on them — and they remain the most useful framework for understanding everyday motion, from cars braking to rockets launching.
The three laws work together: Law 1 defines what "no force" looks like, Law 2 quantifies how force produces acceleration, and Law 3 ensures forces always come in pairs. These laws are the foundation for understanding everything from projectile motion to oscillating springs.
Law 1 — Inertia
An object in motion stays in motion unless acted on by an external force. Friction is an external force: without it, the object never stops.
The Three Laws
Law 1 — The Law of Inertia
An object at rest stays at rest, and an object in motion stays in motion at constant velocity, unless acted upon by a net external force.
Inertia is resistance to change in motion. A heavier object has more inertia. Without friction, a sliding block would never stop — there is no force to change its velocity.
Law 2 — F = ma
The net force on an object equals its mass times its acceleration: F = ma.
| Quantity | Symbol | SI Unit |
|---|---|---|
| Net force | F | Newton (N) |
| Mass | m | kilogram (kg) |
| Acceleration | a | m/s² |
This law is quantitative: doubling the force doubles the acceleration. Doubling the mass halves the acceleration for the same force.
Law 3 — Action and Reaction
For every action there is an equal and opposite reaction.
The forces in Law 3 act on different objects. When you push a wall, the wall pushes back on you with the same force. When a rocket expels gas downward, the gas pushes the rocket upward.
Worked Examples
Worked example
Example 1 — Braking car
A car of mass 1200 kg brakes with a net force of 6000 N. What is its deceleration?
Using F = ma:
The car decelerates at 5 m/s² (i.e. loses 5 m/s of speed every second).
If it was travelling at 20 m/s, it takes:
to come to a complete stop.
Worked example
Example 2 — Rocket thrust and reaction
A rocket engine expels exhaust gas at 3000 m/s and burns 10 kg of fuel per second. What thrust force does the rocket experience?
By Newton's 3rd Law, the thrust equals the reaction force to expelling the exhaust:
The rocket experiences 30 kN of upward thrust, while the exhaust experiences the same force downward.
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