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Eratosthenes measured the Earth with a stick and a shadow

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Around 240 BCE, a librarian in Alexandria worked out the planet's size from the angle of a noon shadow — and got remarkably close.

Verified · Linda Hall Library

Eratosthenes (c. 276–194 BCE), director of the great Library of Alexandria, learned that at noon on the summer solstice the Sun shone straight down a well in Syene (modern Aswan), casting no shadow. At the same moment in Alexandria, to the north, a vertical post cast a shadow at an angle of about 7.2°.

That angle is one-fiftieth of a full circle. Reasoning that the Sun’s rays arrive parallel, he concluded the distance between the two cities must also be one-fiftieth of Earth’s circumference. Multiplying that distance by 50 gave roughly 250,000 stadia.

Because the exact length of his “stadium” is uncertain, scholars can’t pin his error precisely — but his figure lands close to the true circumference of about 40,000 km. With nothing but geometry, shadows and careful measurement, he had sized the whole planet, and proved the Earth’s curvature could be calculated rather than merely assumed.

7.2°
shadow angle
250,000
stadia (his result)
~240 BCE
date

Sources & references

2 references

Well-established. Corroborated by 2 independent sources.

1 Linda Hall Library article “On the longest day of the year, at noon, the Sun is directly overhead in the city of Syene... the shadow angle in Alexandria measured 7.2... 250,000 stadia for the circumference.” lindahall.org ↗
2 Encyclopædia Britannica Encyclopedia “Sunlight fell at an angle of about 7.2 from the vertical... He obtained 250,000 stadia... became director of the great library there.” britannica.com ↗
✓ Last reviewed Jun 6, 2026

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