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The geocentric model assumes a spherical Earth; thus it is not the same as the older flat Earth model. Also, according to this model, the orbits were perfectly circular and not elliptical.
The geocentric model held sway into the early modern age; from the late 16th century onward it was gradually replaced by the heliocentric model of CopernicusNicolaus (or Nicholas Copernicus (original name Kopernik or Koppernigk Polish Mikolaj Kopernik German Nikolaus Kopernikus February 19, 1473 May 24, 1543) was an astronomer, mathematician and an economist who developed a heliocentric ( Sun-centred) theory, GalileoGalileo Galilei ( Pisa, February 15, 1564 Arcetri, January 8, 1642), was a Tuscan astronomer, philosopher, and physicist who is closely associated with the scientific revolution. His great achievements include perfecting the telescope, a variety of astron and KeplerThis article is about Johannes Kepler the astronomer. For the planned planet-finding space telescope, see Kepler Space Mission. Johannes Kepler ( December 27, 1571 November 15, 1630), a key figure in the scientific revolution, was a German astronomer, mat due to the simplicity and predictive accuracy of that newer model.
In this model, a set of fifty-five concentric crystalline spheres were considered to hold the Sun, the planets, and the stars. These spheres (called deferentsIn the Ptolemaic system of astronomy, the epicycle was a geometric model to explain the variations in speed and direction of the apparent motion of the Moon, Sun, and planets. It was designed by Apollonius of Perga at the end of the 3rd century BC. In par) revolved at varying velocities around the Earth to account for the rising and setting of celestial objects every day.
However, this simple model of the revolutions of spheres could not explain all astronomical phenomena. In particular, certain celestial bodies were observed to wander across the fixed fields of stars over time; mostly they wandered in one direction, but occasionally they seemed to reverse course. These "wandering stars" were given the name "planet", based on the Greek word planetes, meaning "wanderer". To explain this strange retrogradationThis article is about retrograde motion. For the musical term retrograde see Counterpoint, Musical set theory, Operation, Permutation, and Transformation. Retrograde motion is the orbital motion of a body in a direction opposite that which is normal to sp, Aristotle claimed that planets were attached, not directly to deferents, but to smaller spheres called epicyclesIn the Ptolemaic system of astronomy, the epicycle was a geometric model to explain the variations in speed and direction of the apparent motion of the Moon, Sun, and planets. It was designed by Apollonius of Perga at the end of the 3rd century BC. In par. The epicycles were themselves attached to the deferents; the simultaneous revolution of both sets of spheres created an occasional apparent reversal of the planets' motions across the skies of the Earth.
Ptolemy further modified this model to more accurately reflect observations by placing epicycles upon epicycles, creating an extraordinarily complicated--but fairly accurate--depiction of the cosmos. He also displaced the Earth from the center of the universe, claiming that, while Earth was enclosed by the celestial spheres, the spheres actually revolved around a point called an eccentric, which was near the Earth but not quite on it.This elaborate theoretical system stemmed largely from one important observation. If Earth did move, then one ought to be able to observe the shifting of the fixed stars due to parallax. In short, the shapes of the constellations should change considerably over the course of a year. In reality, the stars are so very much further away than the sun and the planets that this motion (which does exist) is undetectable without careful telescopic observations using modern equipment, but the lack of any observable parallax was considered the death of any non-geocentric theory for a thousand years.
This view of a geocentric universe held sway for well over a millennium, until the publication of Copernicus's De Revolutionibus Orbium Coelestium in 1543.
In December 1610, Galileo Galilei used his telescope to show that Venus went through phases, just like the moon. This observation was incompatible with the Ptolemaic system. In the 4th century BC, Heraclides Ponticus had already proposed that both Venus and Mercury orbited the Sun rather than Earth. The observation by Galileo led to interest in the more accurate (but still geocentric) Tychonian system, and the heliocentric Copernican system, which both explain how the Sun is commonly in between the Earth and Venus (see Phases of Venus ).
At this time, geocentrism is rejected in scientific and popular opinion; and it is believed that the Sun is at the centre of the solar system, but not the universe (see Heliocentrism). A small number of people still advance a geocentric model (see modern geocentrism). These people tend to be of a religious mindset and sometimes Creationists, because without the concept of God willing to create the Earth at the center of the universe, it would appear mysterious for it to be so.
The geocentric (Ptolemaic) model of the solar system is also of interest to planetarium makers, as for technical reasons a Ptolemaic-type motion for the planet light apparatus has some advantages over a Copernican-type motion.