Biography

Greek astronomer and mathematician of Antiquity, born on the island of Samos. He was the first to propose a heliocentric model placing the Sun, rather than the Earth, at the center of the known world.

Aristarchus

Aristarchus

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SciencesAstronomeMathématicien(ne)Before ChristHellenistic period, 3rd century BCE, at the height of Greek science around Alexandria
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Frequently asked questions

The key thing to remember is that Aristarchus of Samos was a Greek astronomer and mathematician of the 3rd century BC, active in Alexandria, and that he was the first known scholar to propose a heliocentric model, placing the Sun at the centre of the universe and the Earth in orbit around it. This idea, formulated nearly eighteen centuries before Copernicus, is reported by Archimedes in The Sand Reckoner. What is striking here is that his hypothesis, though correct, was rejected by his contemporaries, who preferred geocentrism. Aristarchus is therefore a brilliant but overlooked forerunner of modern astronomy.

Key Facts

  • Born around 310 BCE on the island of Samos, died around 230 BCE
  • First known scholar to propose a heliocentric system (the Earth revolves around the Sun)
  • Author of the treatise On the Sizes and Distances of the Sun and Moon, in which he attempts to measure these distances using geometry
  • His heliocentric ideas, reported by Archimedes, were rejected and forgotten until Copernicus in the 16th century
  • A lunar crater bears his name today in his honor

Works & Achievements

On the Sizes and Distances of the Sun and Moon (3rd century BC)

The only surviving work of Aristarchus, in which he geometrically calculates the relative sizes and distances of the Sun and the Moon. The first known attempt to measure these quantities through reasoning.

Heliocentric hypothesis (lost work) (c. 270 BC)

A now-lost treatise in which Aristarchus placed the Sun at the centre of the world and the Earth in orbit around it. Known only through the testimony of Archimedes.

Measuring the ratio of the Earth-Moon and Earth-Sun distances (3rd century BC)

A method based on observing the Moon at first quarter. Although numerically imprecise, its geometric logic was perfectly correct.

Estimating the sizes of the Sun and Moon (3rd century BC)

Aristarchus concluded that the Sun is far larger than the Earth, an argument that logically led him to place it at the centre rather than the Earth.

Improvement of the sundial (scaphe) (3rd century BC)

An improvement to a hemispherical sundial, attributed by Vitruvius to Aristarchus, allowing one to read the time and the season.

Anecdotes

Aristarchus proposed that the Earth revolves around the Sun nearly eighteen centuries before Copernicus. His idea was so unsettling to his contemporaries that it remained marginal: almost all Greek astronomers continued to place the Earth at the center of the world.

To measure the Earth-Sun distance, Aristarchus had a brilliant idea: at the moment when the Moon is exactly half-lit, he observed the angle between the Sun and the Moon. His method was sound, but his instruments too imprecise: he found a Sun 19 times farther away than the Moon, whereas it is in reality nearly 400 times farther.

The scholar Archimedes, in his treatise *The Sand Reckoner*, explicitly reports that Aristarchus wrote a book placing the Sun at the center and the Earth in orbit around it. It is thanks to this testimony from Archimedes that we know of Aristarchus's heliocentric ideas, for his own work on the subject has been lost.

The Stoic philosopher Cleanthes held that Aristarchus should have been prosecuted for impiety, since moving the Earth from the center of the world amounted, in his view, to “disturbing the rest of the hearth of the universe.” It is one of the oldest known examples of a conflict between a scientific idea and religious beliefs.

Aristarchus understood that the stars do not appear to move when the Earth shifts position, and he deduced that they must lie at immense distances, almost infinite, compared with the Earth's orbit. This intuition of a gigantic cosmos was extraordinarily ahead of its time.

Primary Sources

Archimedes, The Sand Reckoner (c. 250 BC)
Aristarchus of Samos brought out a book consisting of certain hypotheses [...] according to which the fixed stars and the Sun remain unmoved, while the Earth revolves about the Sun on the circumference of a circle, the Sun lying in the middle of the orbit.
Aristarchus, On the Sizes and Distances of the Sun and Moon (3rd century BC)
When the Moon appears to us halved, the distance of the Sun from the Moon is less than a quarter of a circle by one thirtieth of that quarter.
Plutarch, On the Face Which Appears in the Orb of the Moon (c. AD 100)
Cleanthes thought that the Greeks ought to have charged Aristarchus of Samos with impiety for setting in motion the hearth of the universe, supposing that the heavens remain at rest while the Earth moves along an oblique circle and at the same time rotates about its own axis.

Key Places

Island of Samos

Greek island in the Aegean Sea, the homeland of Aristarchus. It had already given birth to the mathematician Pythagoras.

Alexandria

Great Hellenistic city of Egypt, home to the Library and the Museum, where Aristarchus is thought to have studied and worked alongside the greatest scholars.

Athens

Intellectual heart of Greece where Aristarchus is believed to have been trained, notably in the tradition of the Lyceum founded by Aristotle.

Aegean Sea

A maritime expanse dotted with Greek islands connecting Samos to the rest of the Hellenistic world, through which scholars and ideas flowed.

Liens externes & ressources

Œuvres

Sur les grandeurs et les distances du Soleil et de la Lune

IIIe siècle av. J.-C.

Hypothèse héliocentrique (ouvrage perdu)

vers 270 av. J.-C.

Mesure du rapport des distances Terre-Lune et Terre-Soleil

IIIe siècle av. J.-C.

Estimation des tailles du Soleil et de la Lune

IIIe siècle av. J.-C.

Perfectionnement du cadran solaire (scaphé)

IIIe siècle av. J.-C.

Give them back their memoryCharactorium is also a game on Pi Network: revive the forgotten figures of History, one at a time.Play in Pi

See also