Conservation of Energy
Energy cannot be created or destroyed, only transformed.
Formula
Variables
Example
A falling ball trades potential energy for kinetic energy; the total stays constant.
How it works
The conservation of energy tells us that in a closed system, the total amount of energy stays the same even though it can change form, such as from motion to heat or from chemical to electrical energy. This works because energy is a bookkeeping quantity: interactions can move it around or convert it, but they do not make it appear from nothing or vanish on their own. In physics, this principle is deeply connected to the symmetry of nature in time, and it is one of the most reliable tools for predicting how systems behave.
When to use it
Use this formula when you want to track how energy changes in a system without being lost to the outside, such as in mechanics, circuits, heat transfer, or chemical processes. It is especially useful for finding speeds, heights, temperatures, or amounts of work when different energy forms are involved.
Worked example, step by step
A 2.0 kg cart starts at rest at the top of a ramp 5.0 m high and rolls down without friction. Initial gravitational potential energy: E_initial = mgh = (2.0)(9.8)(5.0) = 98 J At the bottom, the cart's potential energy is taken as 0 J, so all of the energy is kinetic. By conservation of energy: E_total = constant, so KE_final = 98 J Use KE = 1/2 mv^2: 98 = 1/2(2.0)v^2 98 = v^2 v = 9.9 m/s Final answer: the cart reaches the bottom with a speed of 9.9 m/s.
Common mistakes to avoid
- Forgetting that energy conservation applies to the whole system, not necessarily to one object alone
- Mixing up energy forms and treating potential energy as if it were always gravitational potential energy
- Ignoring energy losses like friction, air resistance, or heat when the problem says the system is not perfectly isolated
Did You Know?
Energy is never created or destroyed — it only changes form, from chemical to kinetic to heat.
Share this formula
More in Physics Laws & Theorems
View allNewton's First Law (Inertia)
BasicAn object stays at rest or in uniform motion unless acted on by a net force.
Newton's Second Law
BasicNet force equals mass times acceleration (rate of change of momentum).
Newton's Third Law
BasicFor every action there is an equal and opposite reaction.
Conservation of Momentum
IntermediateTotal momentum of an isolated system stays constant.
Archimedes' Principle
IntermediateBuoyant force equals the weight of fluid displaced.
Pascal's Law
IntermediatePressure applied to a confined fluid transmits equally in all directions.