Newton’s Three Laws of Motion, Explained With Everyday Examples
Newton’s first, second and third laws of motion explained simply, with everyday examples, the F = ma formula, worked problems and common misconceptions.
Momentum explained simply: p = mv, conservation of momentum in collisions and explosions, impulse and why crumple zones and airbags work, with worked examples.

Momentum describes how hard it is to stop a moving object. A slow truck and a fast baseball can both be hard to stop, for different reasons.
p = m × v
Because velocity has direction, momentum does too: it’s a vector.
In a closed system with no external forces, total momentum stays the same. This lets you predict what happens in collisions and explosions.
A 1,000 kg car at 10 m/s hits a stationary 1,500 kg car and they move together. Before: 1,000 × 10 = 10,000 kg·m/s. After: (1,000 + 1,500) × v = 10,000, so v = 4 m/s.
When a skater throws a heavy ball forwards, they move backwards: the momenta are equal and opposite. This is Newton’s third law in action; see Newton’s laws of motion.
Impulse = force × time = change in momentum. For the same change in momentum, a longer impact time means a smaller force. That’s why:
Momentum is conserved in both. See kinetic vs potential energy for the energy side.
Kilogram metres per second (kg·m/s), equivalent to newton-seconds (N·s).
No. Inertia is resistance to changes in motion (related to mass); momentum depends on both mass and velocity.
In a closed system with no external forces, yes.
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Newton’s first, second and third laws of motion explained simply, with everyday examples, the F = ma formula, worked problems and common misconceptions.
Kinetic and potential energy explained: formulas, units, everyday examples, energy conversion on roller coasters and pendulums, and a quick energy calculator.
What centripetal force is, the formula F = mv²/r, what provides it in cars, planets and fairground rides, why “centrifugal force” feels real, and examples.