Watch: The Story of Eratosthenes

Before GPS, before satellites, before modern technology - one brilliant mind figured out how to measure our entire planet using only shadows, geometry, and ingenuity.

Watch Carl Sagan explain Eratosthenes

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Who Was Eratosthenes?

Portrait of Eratosthenes of Cyrene

Eratosthenes of Cyrene
(c. 276–195 BCE)

Eratosthenes of Cyrene (c. 276–195 BCE) was an Ancient Greek polymath renowned for his contributions to mathematics, geography, poetry, astronomy, and music theory. As chief librarian at the famous Library of Alexandria in Egypt, he is often called the "Father of Geography" and made numerous contributions to science.

276 BCE

Born in Cyrene (modern-day Libya)

~245 BCE

Appointed chief librarian at the Library of Alexandria

~240 BCE

Wrote Geographika and coined the term "Geography"

Eratosthenes instructing a scholar in Alexandria

As the chief librarian at Alexandria's Library, Eratosthenes advanced geographical studies by introducing enduring terminology and creating the first global map with parallels and meridians — the same coordinate system we use today with GPS!

Image: Eratosthenes instructing a scholar in Alexandria

~240 BCE

Calculated Earth's circumference with remarkable accuracy

~220 BCE

Cataloged 675 stars and calculated the tilt of Earth's axis

194 BCE

Died in Alexandria at approximately 82 years old

Fun Fact: Eratosthenes also invented the "Sieve of Eratosthenes" - an algorithm for finding prime numbers that is still taught in computer science today!

The Library of Alexandria

The Library of Alexandria, built during the early Ptolemaic Dynasty of Egypt, where Eratosthenes served as chief librarian


The World According to Eratosthenes (220 BC)

Eratosthenes is attributed with devising the first system of Latitude and Longitude. He produced this map based on his own calculations and reports from explorers like Nearchus and Pytheas.

Facsimile of the world map by Eratosthenes (around 220 BC)
Map Description: This facsimile shows the known world around 220 BC. It includes place names like Hellas (Greece), Pontus Euxinus (Black Sea), Taprobane (Sri Lanka), and Brettania (Britain). Note the grid lines—Eratosthenes was the first to use such a grid to locate places on Earth. The map highlights his birthplace Cyrene (Libya) and the Egyptian cities Alexandria and Syene (Aswan) pivotal to his circumference calculation.
Source: University of South Florida - Maps ETC

The Brilliant Method

Eratosthenes learned that in the city of Syene (modern-day Aswan, Egypt), on the summer solstice at noon, the sun was directly overhead - so directly that it shone straight down into a deep well without casting any shadow. The sun's rays were perfectly vertical.

However, in Alexandria, where Eratosthenes lived (about 800 km north of Syene), the sun was NOT directly overhead on that same day. Objects cast shadows.

His Key Insight

If the Earth were flat, the sun would cast the same shadow (or no shadow) everywhere. But since Earth is a sphere, the sun's rays hit different parts at different angles!

The Geometry

On the summer solstice at noon:

  • Syene: Sun directly overhead (0° shadow angle)
  • Alexandria: Sun casts shadow at ~7.2° angle
  • Distance between cities: ~5,000 stadia (~800 km)
Geometric diagram of Eratosthenes' measurement

Geometric Representation: The sun's rays are parallel. Angle φ (phi) measured at Alexandria (A) by the shadow is equal to the central angle at the Earth's center. S represents Syene (Aswan). (Source: Wikipedia)

The Calculation

Eratosthenes reasoned:

Circumference = Distance × (360° / Angle)
= 5,000 stadia × (360 / 7.2) = 250,000 stadia

How Accurate Was He?

Converting ancient units to modern measurements is tricky, but most historians estimate:

Measurement Value
Eratosthenes' Result ~39,375 - 46,250 km*
Actual Earth Circumference 40,075 km (equatorial)
Accuracy Within 2-15% of actual value!

*Depending on which definition of "stadion" is used

Remarkable Achievement: Using only a stick, shadows, and his brilliant mind, Eratosthenes calculated the size of our planet to within a few percent of the actual value - over 2,200 years before satellites!

From Shadows to Satellites

In this GPS workshop, you will recreate Eratosthenes' experiment using modern technology:

Eratosthenes (240 BCE) Your Experiment (Today)
Measured shadow angles Measure GPS coordinates
Hired someone to pace distance Pace distance yourself (count steps)
Used geometry to find angular difference Use latitude difference from GPS
Calculated circumference using ratio Calculate circumference using same formula!

The Same Math, New Tools: The fundamental principle is identical - if you know a distance and the corresponding angle of Earth's curvature, you can calculate the whole circumference. Eratosthenes used the sun; you'll use GPS satellites orbiting 20,000 km above Earth!

Why This Matters

Ready to try it yourself? Head to the Field Testing page to conduct Experiment 3: Calculate Earth's Circumference using your GPS unit!

🔧 Don't Have a Working Arduino GPS Unit?

No worries! You can still complete this lab using one of these alternatives:

  • Web-Based GPS App: Use the GPS Web App on any device with GPS capabilities (laptop, tablet, or phone)
  • Commercial GPS Unit: If you have a handheld Garmin, Magellan, or similar device
  • Smartphone GPS App: Download any GPS app that displays your coordinates (e.g., GPS Status, Compass, or your phone's built-in Maps app)

The key is obtaining accurate latitude readings at two different locations — the tool doesn't matter!