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 ↓Each scientist stood on the shoulders of the one before — and each new experiment broke the old model. Click a milestone to jump there.
John Dalton · English schoolteacher & chemist · "Billiard Ball" model
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.
J.J. Thomson · Discovered the electron using cathode ray tubes · Nobel Prize 1906
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!
Ernest Rutherford · The Gold Foil Experiment · "It was as if you fired a shell at tissue paper and it came back and hit you"
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.
Niels Bohr · Fixed energy levels & quantum jumps · Nobel Prize 1922
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.
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!
Erwin Schrödinger & Werner Heisenberg · The model we still use today
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.
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.
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.
| Charge | +1 (positive) |
| Mass | 1 u (heavy) |
| Location | Nucleus |
| Discovered by | Rutherford, 1917 |
| Superpower | Its count = atomic number, which decides WHICH element the atom is! |
| Charge | 0 (neutral) |
| Mass | 1 u (heavy) |
| Location | Nucleus |
| Discovered by | Chadwick, 1932 |
| Superpower | Nuclear glue! Changing its count makes isotopes of the same element. |
| Charge | −1 (negative) |
| Mass | ≈ 1/1836 u (super light!) |
| Location | Shells / orbitals around nucleus |
| Discovered by | Thomson, 1897 |
| Superpower | Runs all of chemistry — bonding, electricity and light all come from electrons. |
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!).