The Story of the Atom

How did we figure out what everything is made of — without ever seeing an atom? Travel through 120 years of brilliant experiments, wrong turns and eureka moments. Every model below is interactive: click, drag and run the experiments yourself.

Begin the Journey ↓
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Five Models. One Century.

Each scientist stood on the shoulders of the one before — and each new experiment broke the old model. Click a milestone to jump there.

Dalton1803 · Solid Sphere
Thomson1897 · Plum Pudding
Rutherford1911 · Nuclear
Bohr1913 · Planetary
Schrödinger1926 · Quantum Cloud
1803

The Solid Sphere Model

John Dalton · English schoolteacher & chemist · "Billiard Ball" model

Try it: Atoms as tiny solid balls

Dalton imagined atoms as hard, indivisible spheres — like microscopic billiard balls, constantly moving and bouncing. Different elements = different sized balls.

Add atoms, switch elements (notice the size changes!) and crank up the heat to watch them race around. Atoms of the same element are identical — atoms of different elements differ.

What Dalton got right

  • All matter is made of atoms — tiny particles too small to see.
  • Atoms of one element are identical, and different from atoms of other elements.
  • Atoms combine in fixed whole-number ratios to form compounds (like H₂O — always 2:1!).
  • Atoms can't be created or destroyed in chemical reactions — only rearranged.
The crack in the model: Dalton said atoms are indivisible — but in 1897, Thomson found something smaller hiding inside them…
1897

The Plum Pudding Model

J.J. Thomson · Discovered the electron using cathode ray tubes · Nobel Prize 1906

Try it: Electrons in a positive "pudding"

Thomson discovered electrons — tiny negative particles nearly 2000× lighter than the whole atom. He pictured them stuck inside a ball of positive charge, like plums in a pudding.

Drag the electrons around inside the pudding — they're free to move, but can't escape the positive sphere. Then run the actual experiment that discovered them!

The discovery that changed everything

  • The cathode ray experiment: a mysterious glowing beam inside a vacuum tube bent toward the positive plate — proving the beam was made of negative particles.
  • Atoms are divisible after all! Electrons are pieces of atoms — Dalton's "indivisible" ball was broken open.
  • Atoms are neutral overall, so positive charge must exist to balance the negative electrons.
The crack in the model: Where exactly is the positive charge? Thomson guessed it was spread out like pudding. His own student was about to prove him spectacularly wrong…
1911

The Nuclear Model

Ernest Rutherford · The Gold Foil Experiment · "It was as if you fired a shell at tissue paper and it came back and hit you"

Try it: A tiny nucleus in empty space

Rutherford pictured the atom as mostly empty space: a tiny, dense, positive nucleus at the centre, with electrons whirling far around it. He proved it by firing positive alpha particles at ultra-thin gold foil — if Thomson's pudding were right, they should all sail straight through.

This is Rutherford's nuclear model. Notice how tiny the nucleus is compared to the whole atom — and it's still drawn thousands of times too big! Now run the experiment that revealed it.

What the experiment proved

  • Atoms are mostly empty space — that's why almost all alpha particles passed straight through.
  • A tiny, dense, positive nucleus sits at the center — only a direct hit made particles bounce back.
  • Scale check: if an atom were a football stadium, the nucleus would be a marble at the center field!
  • Electrons orbit somewhere in the empty space around the nucleus.
The crack in the model: Physics said an orbiting electron must constantly lose energy and spiral into the nucleus in 0.00000001 seconds. Atoms shouldn't exist! Yet they do. Enter: Niels Bohr…
1913

The Planetary Model

Niels Bohr · Fixed energy levels & quantum jumps · Nobel Prize 1922

Try it: Make the electron jump!

Bohr's fix: electrons can only ride on fixed orbits (energy levels), like rungs of a ladder. They never spiral in — they can only jump between levels by absorbing or releasing light.

Energy level: n = 1Photon: —

You can also click directly on any orbit to send the electron there. Falling from higher levels releases photons of different colours — this is exactly why neon signs and fireworks glow in specific colours!

Why this model was genius

  • Electrons live on fixed energy levels (n = 1, 2, 3…) — they can't exist in between.
  • Jump up = absorb energy. Fall down = emit light of an exact colour.
  • It explained the hydrogen spectrum perfectly — the exact colours hydrogen gas glows had puzzled scientists for decades.
  • Atoms are stable because an electron on the lowest rung (n = 1) has nowhere lower to fall.
The crack in the model: It only worked for hydrogen (1 electron). For every other element, the maths failed. And electrons, it turns out, don't move in neat circles at all…
1926

The Quantum Cloud Model

Erwin Schrödinger & Werner Heisenberg · The model we still use today

Try it: Hunt the electron

In the modern model, an electron has no fixed path. We can only know the probability of finding it somewhere. The fuzzy cloud below shows where the electron is likely to be — denser cloud = higher chance.

Showing: 1s orbital — a simple sphere of probability

Press "Measure" repeatedly — the electron appears in a different random spot each time, but almost always inside the dense part of the cloud. That IS the orbital: a map of probability, not a path.

The model we use today

  • Electrons behave like waves, not tiny planets. Schrödinger's equation describes their wave.
  • Heisenberg's Uncertainty Principle: you can never know an electron's exact position and speed at the same time.
  • Orbitals replace orbits — 3D regions (s, p, d, f) where the electron is most likely to be found.
  • It works for every element — and powers all of modern chemistry, lasers, LEDs and computer chips.
The story isn't over: in 1932 Chadwick found the neutron, and today we know protons and neutrons are made of even smaller quarks. Science never stops asking "what's inside?"

⚛ The Particle Lab

Meet the three particles that build every single thing in the universe — then use them to build your own atoms. Tap each card to flip it.

p⁺

Proton

Positive · lives in the nucleus
tap to flip ↻

Proton

Charge+1 (positive)
Mass1 u (heavy)
LocationNucleus
Discovered byRutherford, 1917
SuperpowerIts count = atomic number, which decides WHICH element the atom is!
n⁰

Neutron

Neutral · lives in the nucleus
tap to flip ↻

Neutron

Charge0 (neutral)
Mass1 u (heavy)
LocationNucleus
Discovered byChadwick, 1932
SuperpowerNuclear glue! Changing its count makes isotopes of the same element.
e⁻

Electron

Negative · orbits the nucleus
tap to flip ↻

Electron

Charge−1 (negative)
Mass≈ 1/1836 u (super light!)
LocationShells / orbitals around nucleus
Discovered byThomson, 1897
SuperpowerRuns all of chemistry — bonding, electricity and light all come from electrons.

🔬 Build-an-Atom

Add or remove particles and watch your atom change identity, mass and charge in real time.

Electrons fill shells from the inside out: 2 → 8 → 8 (the rule you learn in class!).

Protons
1
Neutrons
0
Electrons
1
H
Hydrogen
Atomic number: 1 Mass number: 1 Neutral atom
The simplest atom in the universe ✨