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06 / ANTIQUITY TO THE RENAISSANCE

Eratosthenes of Cyrene

c. 276–194 BCE·Cyrene · Alexandria

You can measure a whole planet without travelling all the way around it. Measure one part, then find how many copies make a full turn.

Explore the mathematics ↓
Imagined portrait of Eratosthenes of Cyrene
Imagined likeness

01 / A PART AND THE WHOLE

Measure the Earth with a shadow

At noon on midsummer’s day, the sun stood straight above Syene: upright sticks cast no shadow. At the same moment in Alexandria, a stick cast a short one.

That little shadow angle is the key. Because sunlight is parallel, it tells you what slice of the whole Earth lies between the two cities.

Why does one stick cast a shadow and the other not?

At noon in Syene the sun is straight overhead. Drag City B along the Earth and watch its stick’s shadow.

Earth shown in cross-section · city markers, sticks and shadows enlarged
Route from Syene to City B?
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Copies to go all the way round?
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Earth’s circumference?

Eratosthenes’ own numbers

He reportedly measured 7.2° at Alexandria, one fiftieth of a full turn, and took the route to Syene as 5,000 stadia.

So the Earth is 50 × 5,000 = 250,000 stadia around. The exact length of his stadium is debated, so the lesson uses modern kilometres.

THE IDEAThe shadow angle at the stick equals the angle at Earth’s centre. If it is 1/50 of a full turn, the route is 1/50 of the way around the Earth.

The person behind the ideas

More of the mathematics

The sieve of Eratosthenes

Crossing out multiples systematically leaves the prime numbers: numbers greater than 1 with no smaller whole-number factors except 1.

Mathematical geography

He connected distances, latitude, and a spherical Earth to the task of making maps.