Eratosthenes(275 av. J.-C. — 193 av. J.-C.)

Eratosthenes

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SciencesLiteraturePhilosophyAstronomeBefore ChristHellenistic period, 3rd – 2nd century BC

Greek scholar of the 3rd century BC and director of the Library of Alexandria. He measured the circumference of the Earth with remarkable accuracy and laid the foundations of scientific geography.

Frequently asked questions

Eratosthenes was a Greek scholar of the 3rd century BC, director of the Library of Alexandria. He is famous for measuring the circumference of the Earth with remarkable accuracy, finding about 40,000 km — a value very close to the real one. He also invented the Sieve of Eratosthenes, a method for finding prime numbers still used today. What you should remember is that he was a versatile genius, nicknamed “Beta” because he excelled in many fields without being first in any single one.

Key Facts

  • Around 275 BC: born in Cyrene (present-day Libya)
  • Around 245 BC: appointed director of the Library of Alexandria by Ptolemy III
  • Around 240 BC: measured the circumference of the Earth by comparing the angles of shadows in Alexandria and Syene, obtaining a result close to the actual value (~40,000 km)
  • Invented the 'Sieve of Eratosthenes', a method for finding prime numbers
  • Around 193 BC: died in Alexandria, probably around the age of 80

Works & Achievements

Geographica (Vers 240-220 av. J.-C.)

Premier traité systématique de géographie mathématique, dans lequel Ératosthène décrit le monde habitable, calcule la circonférence de la Terre et introduit un système de coordonnées géographiques. L'œuvre originale est perdue mais connue par les citations de Strabon.

Sur la mesure de la Terre (Vers 240 av. J.-C.)

Traité décrivant sa méthode géodésique pour mesurer la circonférence terrestre à partir de l'angle solaire entre Alexandrie et Syène, aboutissant à une estimation d'environ 40 000 km.

Chronographies (Vers 220-200 av. J.-C.)

Œuvre fondatrice de la chronologie historique grecque, dans laquelle Ératosthène tenta d'établir une datation précise des grands événements depuis la guerre de Troie, posant les bases de l'histoire comme science.

Catastérismes (IIIe siècle av. J.-C.)

Recueil mythologique associant les constellations aux légendes grecques, qui influença durablement la nomenclature astronomique. Son attribution à Ératosthène reste discutée mais plausible.

Le Crible d'Ératosthène (méthode arithmétique) (IIIe siècle av. J.-C.)

Algorithme permettant d'identifier tous les nombres premiers inférieurs à un nombre donné par élimination successive des multiples. C'est l'une des plus anciennes méthodes algorithmiques connues, encore utilisée en informatique.

Anecdotes

To measure the circumference of the Earth, Eratosthenes used an ingenious method: in Syene (modern-day Aswan), the sun shone directly down to the bottom of wells at noon on the summer solstice, while in Alexandria, about 800 km to the north, it cast a shadow. By measuring this angle of approximately 7.2°—one-fiftieth of a full circle—he calculated Earth's circumference at roughly 40,000 km, a remarkably accurate result.

Eratosthenes was nicknamed 'Beta' by his contemporaries because he excelled across many disciplines without ever being considered the greatest in any single one. Some saw this as a criticism, but others interpret the nickname as recognition of exceptional versatility: he was a mathematician, geographer, astronomer, poet, and philosopher all at once.

He invented the 'Sieve of Eratosthenes,' a method for finding all prime numbers up to a given value by successively eliminating the multiples of each number. This simple and elegant technique is still taught today in mathematics classrooms around the world.

Eratosthenes was appointed by King Ptolemy III as director of the famous Library of Alexandria, the largest collection of knowledge in the ancient world. There he gathered and organized papyrus scrolls from across the Mediterranean, personally overseeing the creation of a monumental catalogue known as the Pinakes.

Primary Sources

Strabo's Geography (excerpts on Eratosthenes) (1st century BC)
Eratosthenes says that the Earth is a sphere, not perfectly round like a ball, but presenting certain irregularities. He estimated its circumference at 252,000 stades, based on the observation that Syene and Alexandria are 5,000 stades apart.
On the Nature of the Gods — Cleomedes, On the Circular Motions of the Celestial Bodies (4th century AD (reporting older sources))
Eratosthenes measured the size of the Earth using a mathematical method and obtained a result of 250,000 stades. He assumed that Syene lies on the Tropic of Cancer, and that in Alexandria, at the same hour, the sun casts a shadow at an angle of one-fiftieth of a circle.
Eratosthenes' Chronographies (fragments cited by Apollodorus of Athens) (3rd century BC)
Eratosthenes established a chronology of events from the Trojan War to his own time, setting the date of the fall of Troy at 1183 BC, thereby laying the foundations of Greek historical chronology.
Eratosthenes' Geographica (fragments reconstructed by H. Berger, 1880) (3rd century BC)
He drew a map of the inhabited world (oikoumene) drawing on the accounts of travelers and navigators, introducing for the first time a system of parallel lines and meridians to locate places.

Key Places

Cyrene (modern-day Shahhat, Libya)

Eratosthenes' birthplace, a prosperous Greek colony on the North African coast renowned for its philosophers and scholars. He received his early intellectual education there before moving to Athens.

Athens

Eratosthenes studied in Athens at the great philosophical schools of the time, notably under the philosopher Arcesilaus at the Academy, before being invited to Alexandria.

Alexandria (Egypt)

The intellectual capital of the Hellenistic world, where Eratosthenes spent most of his life directing the famous Library and the Mouseion, the great center of ancient knowledge.

Syene (modern-day Aswan, Egypt)

A city located on the Tropic of Cancer, where Eratosthenes observed that the sun stood directly overhead at noon on the summer solstice. This geographical reference point was crucial to his measurement of the Earth.

See also