Two Shadows Helped Measure the Whole Earth
More than two thousand years ago, a Greek scholar named Eratosthenes worked in the great library in Alexandria, in Egypt. He heard about a deep well in a southern town called Syene. On one day each summer, at noon, sunlight shone straight down the well and lit the water at the bottom. This meant that the sun was directly overhead in Syene at that moment.
Eratosthenes wondered about the same day in Alexandria. He set up a tall pole and watched its shadow at noon. The pole did cast a shadow, which meant the sun was not straight overhead there. He measured how far the sun's rays tilted from the pole, and it was about one fiftieth of a full circle.
Here is the clever part. Sunlight reaches Earth in nearly parallel rays. If the ground were flat, the two towns would have the same shadows. Different shadows meant the surface curved between them. The angle of the shadow matched the curve of Earth between the two places.
Eratosthenes knew roughly how far apart the towns were, because surveyors had paced it off. If that distance was one fiftieth of the way around Earth, then the whole trip had to be fifty times longer. He multiplied, and he got a number for the size of the planet.
His answer was surprisingly close to what we know today. He used only a pole, the sun and good thinking.