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.
Kinetic and potential energy explained: formulas, units, everyday examples, energy conversion on roller coasters and pendulums, and a quick energy calculator.

Energy is the ability to do work, and in mechanics it comes in two main forms: energy of motion and stored energy. Understanding how they convert explains everything from roller coasters to bouncing balls.
Kinetic energy (KE) is the energy an object has because it’s moving:
KE = ½ m v²
Because speed is squared, doubling speed quadruples kinetic energy, which is why car crashes at higher speeds are so much more dangerous.
Gravitational potential energy (PE) is energy stored because of an object’s height:
PE = m g h
Other forms of potential energy include elastic (stretched springs) and chemical (fuel, food).
In reality, some energy is lost to air resistance, friction and sound; see friction explained.
A 2 kg ball dropped from 10 m (ignoring air resistance): PE at the top = 2 × 9.81 × 10 = 196.2 J. Just before landing, nearly all of this becomes KE, so ½ × 2 × v² = 196.2, giving v ≈ 14 m/s.
For how energy relates to work and power, see work, energy and power.
Yes. A flying plane has kinetic energy from its speed and potential energy from its height.
The joule (J).
Energy is conserved, but it can be transformed into less useful forms, like heat.
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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.
Momentum explained simply: p = mv, conservation of momentum in collisions and explosions, impulse and why crumple zones and airbags work, with worked examples.
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.