Eratosthenes, or rather Eratosthenes of Cyrene (275-194BC), was an ancient Greek scientific writer, mathematician, astronomer and poet (basically a polymath). Born in Cyrene (modern Libya), he was educated at Alexandria and Athens, eventually becoming entrusted with the care of the library at Alexandria. Circa 200BC he developed an algorithm for finding all prime numbers up to a specified integer known as the “Sieve of Eratosthenes.” Myth suggests he inscribed the series of odd numbers on parchment, and then cutting out the composite numbers, the parchment with all its holes resembled a sieve, hence the reason why the algorithm is named Eratosthenes Sieve. However Eratosthenes also invented the Julian calendar, and calculated the circumference of the Earth.

Eratosthenes surmised that in Aswan (Syene) on June 21, the sun would be directly overhead and cast no shadow. At the same moment, the sun would cast shadows in Alexandria, about 600 miles north of Aswan. So at noon on June 21, 230BC, Eratosthenes measured the height of a pole, and the length of its shadow in Alexandria. He found that angle ∠1 measured about 7.2°. Based on the idea that the sun’s rays are parallel, and that “alternate interior angles of parallel lines are congruent”, then ∠1 ≅ ∠2. Therefore ∠2 = 7.2°, or 1/50 of a circle. Assuming the distance between Aswan and Alexandria to be 5000 stades then Eratosthenes found the circumference of the earth (c) to be:
7.2/360 = 5000/c c = 250,000 stades★ 1 stade = 185m c = 46,250km
★ What is a stade? A stade was an ancient Greek unit of length, defined as consisting of 600 Greek feet. There were a bunch of actual sizes for stadia used in the ancient world (possibly six or more), and it is a hotly debated topic.
Engels [2] suggests Eratosthenes used the Attic stade at 184.98m. Although many people have cited the use of the itinerary stade (157m) [3], Engels [2] provides arguments questioning the validity of this number, and why the Attic stade makes sense. One such work is the empirical determination of the length of the stadia made by Lev Vasilevich Firsov, who averaged 81 distances given by Eratosthenes and Strabo with straight-line distances measured by modern methods [4], resulting in a value of 157.7m. One of the arguments is that many authors from the first century AD suggest that 1 Roman mile = 8 stades. A Roman mile is roughly 1480m, so 1/8 of a mile is 185m [1]. Recent work also tends to favour the use of 185m [5].
Now the actual equatorial circumference is 40,075km, so the calculation is not terrible considering the amount of approximation going on (15% difference). Using this value of 157m, the result is 39,250km, which is only a 2% error (and hardly seems believable). The fact that Eratosthenes’s result is not 100% accurate does not distract from the fact that what he achieved was remarkable. There has been at least one modern experiment performed to replicate Eratosthenes’s method [6].
Further Reading:
- Walkup, N., “Eratosthenes and the Mystery of the Stades” Dissertation (2005)
- Engels, D., “The Length of Eratosthenes’ Stade”, American Journal of Philology, 106(3), pp.298-311 (1985)
- Dreyer, J. L. E., “The well of Eratosthenes”, The Observatory, 37, pp.352-353 (1914)
- L. V. Firsov, “Eratosthenes’ Calculation of the Earth’s cumference and the Length of the Hellenistic Stade”, Journal of Ancient History, 121, pp.154-175 (1972)
- Shcheglov, D.A., “The so-called ‚Itinerary Stade‘ and the Accuracy of Eratosthenes’ Measurement of the Earth”, KLIO, 100(1), pp.153-177 (2018)
- Longhorn, M., Hughes, S., “Modern replication of Eratosthenes’ measurement of the circumference of Earth”, Physics Education, 50(2), pp.175-178 (2015)

