科技史宇宙Civiliverse

Idea

Heliocentrism

日心说

Someone suggested more than two thousand years ago that it might be we who move; the idea was then shelved for eighteen centuries.

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The astronomical doctrine placing the Sun, not the Earth, at the center of the cosmos or solar system. The ancient Greek Aristarchus (c. 270 BCE) proposed it and was ignored; Copernicus systematically revived it in De revolutionibus (1543); Kepler set elliptical orbits, Galileo furnished telescopic evidence and angered the Church (tried in 1633), and Newton's mechanics gave it a physical foundation. Copernicus's mathematical models drew heavily on Islamic astronomy (the Maragha school). It is the emblematic opening of the Scientific Revolution.

Date
c. 1543–1687
Place
Europe (heir to Greek and Islamic astronomy)
Civilisation
Western, Greco-Roman, Islamic world
Fields
Astronomy, Geography & Navigation, Natural Philosophy & Method

In the middle of all sits the Sun enthroned… as if upon a royal throne, ruling the family of planets that wheel around him.

—— Copernicus, De revolutionibus, Book I (1543)
The heliocentric diagram in Copernicus's De revolutionibus (1543): the Sun at centre, the planetary orbits ringed around it. An illustration that turned heaven and earth upside down.
The heliocentric diagram in Copernicus's De revolutionibus (1543): the Sun at centre, the planetary orbits ringed around it. An illustration that turned heaven and earth upside down.Nicolaus Copernicus, public domain, via Wikimedia Commons source
Interactive 3D modelEpicycles & heliocentrismOpen this entry in the atlas and choose “Open 3D model”

History

The conjecture of a central Sun did not begin with Copernicus. Around 270 BCE the Greek Aristarchus proposed that the Earth circles and spins about the Sun, but before the authority of the Aristotelian-Ptolemaic geocentric system and the common sense of "if the Earth moved, why do we not feel it," the idea lay buried for a thousand years. In 1543 the Polish canon Copernicus, in De revolutionibus, published on his deathbed, systematically rebuilt the heliocentric model to explain such phenomena as planetary retrogradation. Recent scholarship finds that several of Copernicus's mathematical tools (such as the "Tusi couple") match closely the models of the Islamic Maragha-school astronomers (al-Tusi, Ibn al-Shatir), so that his doctrine in fact inherited the advances of Arab astronomy. Thereafter Kepler, from Tycho's precise observations, set elliptical orbits; Galileo, with the telescope, saw the phases of Venus and the moons of Jupiter, furnishing evidence for heliocentrism—and for it was tried by the Roman Inquisition in 1633 and forced to recant. Only with Newton's universal gravitation did the heliocentric system win a solid physical footing.

Why it matters

What most repays thought in heliocentrism is the fate of Aristarchus: a correct idea proposed eighteen centuries too early, ignored for want of the evidence (the telescope), the mechanics (inertia), and the mathematics (the ellipse) to support it. This echoes the fate of movable type—being "first" in technology or in idea is never the same as being "first" to win in history; whether an idea takes root depends on whether the whole network of conditions to receive it was ready when it arrived. Heliocentrism is also a fine case against Whig history: Copernicus himself was quite conservative, still wedded to perfect circular motion and still using epicycles, a "reluctant revolutionary"; and some of the mathematical tools of this "revolution" came from Islamic astronomy. To enshrine heliocentrism as the myth of "European reason suddenly opening its eyes" wrongs Aristarchus and erases Maragha alike.

Connections

Causes6

Consequences3

Sources

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