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Eratosthenes' Earth Measurement: A Geometric Triumph of Ancient Wisdom

An ancient Greek scholar's ingenious method for measuring the Earth's circumference using basic geometry and shadows.

mysimulator teamUpdated June 2026≈ 3 min read▶ Open the simulation

What Eratosthenes' Experiment Was

Eratosthenes, a polymath from ancient Greece, devised an ingenious method around 240 BC to measure the Earth's circumference. He observed that on the summer solstice at noon, in the city of Syene (modern-day Aswan), a vertical stick cast no shadow because the sun was directly overhead. In Alexandria, about 500 miles north, he noticed a small shadow cast by a similar stick.

By comparing these observations and using basic geometry, Eratosthenes calculated that the angle difference between the two cities' shadows corresponded to approximately one-fiftieth of the Earth's circumference.

Why It Happened

The key to Eratosthenes' method lies in understanding how parallel rays from the sun converge at different angles on the Earth's surface due to its curvature. When the sun is directly overhead, it casts no shadow; as the angle of incidence changes with latitude, shadows are cast.

Eratosthenes used the geometry of triangles and simple trigonometry to relate the angular difference in shadows to the actual distance between the two cities, thereby estimating the Earth's circumference.

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How It Changed Our Understanding

Eratosthenes' experiment was a landmark achievement that demonstrated the vast scale of our planet and laid the groundwork for modern geodesy. His method provided an accurate estimate of Earth's circumference, which was remarkably close to today’s known value.

More importantly, it showcased how precise measurements can be made using simple tools and principles of geometry, inspiring generations of scientists and mathematicians.

Modern Applications

While Eratosthenes' method is no longer used for practical Earth measurements due to more advanced techniques, his approach remains a cornerstone in educational curricula worldwide. It illustrates the power of simple observations and geometric reasoning.

The principles behind his experiment are also relevant in fields like astronomy, where similar methods are used to measure distances in space.

Frequently asked questions

How did Eratosthenes know when the sun was directly overhead?

Eratosthenes knew that on the summer solstice at noon, the sun would be directly overhead in Syene because he had heard from travelers about a well where the sun's rays could reach to the bottom of it during this time.

Why did Eratosthenes choose Alexandria for his second observation point?

Alexandria was chosen as it is approximately 500 miles north of Syene, making it a convenient distance to measure and providing a significant enough angular difference in shadows.

What if the sun's rays were not perfectly parallel?

The assumption that the sun's rays are parallel is valid for practical purposes on Earth because the Sun is so far away. Any slight deviation would result in a small error, but it does not significantly affect the overall accuracy of Eratosthenes' method.

How accurate was Eratosthenes' estimate?

Eratosthenes estimated Earth's circumference to be about 250,000 stadia (a unit of length), which translates to approximately 46,300 kilometers. Modern measurements give the Earth’s circumference as around 40,075 kilometers, showing his estimate was remarkably close.

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