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.
Speed, velocity and acceleration explained: scalars vs vectors, formulas, units, reading distance-time and velocity-time graphs, and worked examples.

Speed, velocity and acceleration describe motion. They’re often confused, but the differences matter in every physics problem.
Speed = distance ÷ time, measured in m/s. It’s a scalar: it has size but no direction.
Velocity = displacement ÷ time, where displacement is the straight-line change in position with direction. It’s a vector. A car driving around a roundabout at a steady 30 km/h has constant speed but changing velocity.
Acceleration = change in velocity ÷ time
a = (v − u) ÷ t
Units: m/s². Slowing down is sometimes called deceleration, a negative acceleration.
| Graph | Slope means | Area means |
|---|---|---|
| Distance–time | Speed | — |
| Velocity–time | Acceleration | Distance travelled |
A flat line on a distance–time graph means stationary; on a velocity–time graph it means constant velocity.
For constant acceleration: v = u + at, s = ut + ½at², v² = u² + 2as. They’re used in our free fall and projectile motion calculators, and they follow from Newton’s second law.
Yes, if its direction changes, as in circular motion; see centripetal force.
No. Velocity can be negative when an object moves in the opposite direction to the one chosen as positive.
Metres per second squared (m/s²).
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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.
Momentum explained simply: p = mv, conservation of momentum in collisions and explosions, impulse and why crumple zones and airbags work, with worked examples.