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Physics Physics

Classical Mechanics · Energy & Work

Energy is the Universe's Bookkeeping

You never see energy directly — you see rocks fall, fires burn, muscles flex. But underneath every transformation is a number that never changes. Conservation of energy is the deepest accounting system in all of physics.

KE · PE · Work · Power 3 Simulations Grades 6–12
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There is a fact, or if you wish, a law, governing all natural phenomena that are known to date. There is no known exception to this law — it is exact so far as we know. The law is called the conservation of energy. It states that there is a certain quantity, which we call energy, that does not change in the manifold changes which nature undergoes.

— Richard Feynman

Idea 1 · What is Energy?

Energy: A Number That Never Changes

Feynman opened with a striking admission: we don't actually know what energy is. It isn't a fluid, a substance, or a thing. It is an abstract quantity — a number — that stays constant no matter what physical processes occur.

Think of a child's "Dennis the Menace" blocks. Mom can always account for all the blocks, even when some are in a box, some in the water, some hidden under the rug. Energy is like that. The universe can store it in different "hiding places" — but the total never changes.

The Conservation Law

Total Energy = Kinetic + Potential + Heat + Electrical + Chemical + Nuclear + ...
This total is always the same. Nature never creates or destroys energy — only converts it between forms.

SI Unit: the Joule (J)

One joule is the energy needed to lift an apple (≈100g) one meter upward against Earth's gravity. A food calorie (kcal) equals 4,184 joules. A lightning bolt delivers about 250 kJ. The Sun radiates 3.8 × 10²⁶ joules every second.

E_total = constant
Noether's Theorem

Conservation of energy isn't arbitrary — it follows mathematically from the fact that the laws of physics are the same today as they were yesterday. Time-translation symmetry implies energy conservation. Emmy Noether proved this in 1915.

Idea 2 · The Two Master Forms (and their children)

Kinetic Energy and Potential Energy

Kinetic Energy — the energy of motion

KE = ½mv²

Every moving object has kinetic energy. It grows with the square of velocity — double the speed means four times the KE. This is why highway crashes are so much more destructive than parking lot fender-benders.

Gravitational Potential Energy

PE = mgh

An object held above the ground has potential energy stored in the gravitational field. When released, gravity converts it to kinetic energy. h is height above a chosen reference point — you can choose any reference, since only changes in PE matter.

Other Forms of Energy

🔥
Thermal
Kinetic energy of randomly moving atoms. Temperature measures the average.
⚗️
Chemical
Potential energy stored in electron bonds between atoms.
Electrical
Energy of charges moving through fields — powers every device.
☀️
Radiant
Energy carried by photons — light, radio, X-rays, gamma rays.
⚛️
Nuclear
Energy in strong/weak nuclear force bonds. E = mc² applies here.
🌊
Elastic
Stored in compressed or stretched materials. PE = ½kx²
⚡ Energy Roller Coaster Watch KE and PE trade back and forth — total energy stays constant
Kinetic (KE)0% Potential (PE)100% Heat Lost0% Total100%

Idea 3 · Work — Transferring Energy Through Force

Work: Force × Distance in the Same Direction

W = F · d · cos(θ)

Work is energy transferred to or from an object by a force acting over a distance. The angle θ is between the force direction and the direction of motion. Only the component of force along the motion does work.

  • Lift a 10 N box 2 m → W = 20 J (θ = 0°, cos0 = 1)
  • Carry a box horizontally → W = 0 J (force is vertical, motion is horizontal)
  • Friction slowing a car → W is negative (force opposes motion)
Work–Energy Theorem

The net work done on an object equals the change in its kinetic energy: W_net = ΔKE = ½mv² − ½mv₀²

Power: Rate of Doing Work

P = W/t = F·v

Power is how fast energy is transferred. Unit: the Watt (W = J/s). A 100 W lightbulb consumes 100 joules every second. A Tour de France cyclist outputs ~400 W sustained. A horse: ~750 W (1 horsepower).

Efficiency

No real machine converts energy perfectly. Some always becomes heat (friction, air resistance). Efficiency = (useful output energy) / (total input energy) × 100%. A car engine: ~25%. A human muscle: ~25%. An LED: ~80%.

Why Can't Efficiency Be 100%?

Thermodynamics limits it. The Second Law says that in every energy conversion, some energy "spreads out" into heat — increasing entropy. A perfectly efficient engine would violate the Second Law of Thermodynamics.

🔧 Work Calculator: Force × cos(θ) Drag the force angle to see how much work is done vs. wasted sideways
Work Done200 J Wasted (⊥)0 J

Idea 4 · Conservative vs. Nonconservative Forces

Path Independence: The Hallmark of Conservation

Conservative Forces

A force is conservative if the work it does is independent of the path taken — only the starting and ending positions matter. Examples: gravity, springs (Hooke's Law), electric force (Coulomb's Law).

For a conservative force, you can define a potential energy function. Going around a closed loop returns you to the same energy state.

W = −ΔPE  (conservative)

Nonconservative Forces

Friction, air resistance, tension — these are nonconservative. The work they do depends on the path; taking a longer path means more energy lost to heat. You can't recover that energy as potential energy — it has spread into thermal motion.

The Full Energy Equation

KE_initial + PE_initial + W_nonconservative = KE_final + PE_final
The nonconservative work term (friction, drag) accounts for energy converted to heat. Total energy is still conserved — it just moves into forms we can't easily use.

Potential Energy Fields

Every conservative force has a potential energy field — a map of stored energy in space. Gravity: PE = mgh. Electric: PE = kq₁q₂/r. Spring: PE = ½kx². Objects "roll downhill" in these fields toward lower potential energy.