Imagine that you are very small. So small that photons of light zoom past, bounce off you, speed you up in the collision. You’re driving a tiny space-ship, in the solar system of a single atom. There is the nucleus—a ball of protons and neutrons the size of a seed—surrounded by an enormous “cloud” of electrons, mostly empty space, which appears to you as big as a football stadium. Your space-ship is an electron, and someone out there in the big world is trying to measure your speed, as you soar through atomic space. This quantum traffic-cop is aiming a speed-gun at you, and he wants to know exactly where you are at this instant, and how fast you’re going. But he discovers, when he tries, that down here in atomic space, motion doesn’t work the way it does in the larger world.
The speed-gun’s ray of light is a stream of photons: particles, objects of light. When the photons bounce off your electron space-ship, back to the gun, they bump you out of place. Even as the traffic-cop reads your location from the bounced-back light particles, you are moved by them. It’s as if the cop is shooting a moving car with a Volkswagen, trying to measure the first car’s position by the ricochet of the second. This is what it’s like to measure an electron.
The year is 1927, the place Copenhagen. The man peering into his imaginary microscope is a brilliant 26-year-old physicist named Werner Heisenberg. Two years earlier, Heisenberg helped develop the math behind quantum mechanics—the equations to explain the laws of the atomic universe, determining how the tiny particles in the atomic solar system move and interact. But the discovery he first voiced in a letter in February 1927 is the one that will carry his name forever: the Heisenberg Uncertainty Principle.