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Jun 14, 2024 · Ptolemaic system, mathematical model of the universe formulated by the Alexandrian astronomer and mathematician Ptolemy about 150 CE. The Ptolemaic system is a geocentric cosmology that assumes Earth is stationary and at the centre of the universe.
- Geocentric model | Definition, History, & Facts | Britannica
Geocentric model, any theory of the structure of the solar...
- Ptolemy's geocentric model of the solar system | Britannica
The most important solution to this problem was proposed by...
- Geocentric model | Definition, History, & Facts | Britannica
In astronomy, the geocentric model (also known as geocentrism, often exemplified specifically by the Ptolemaic system) is a superseded description of the Universe with Earth at the center. Under most geocentric models, the Sun, Moon, stars, and planets all orbit Earth.
May 1, 2024 · Geocentric model, any theory of the structure of the solar system (or the universe) in which Earth is assumed to be at the center of it all. The most highly developed geocentric model was that of Ptolemy of Alexandria (2nd century CE).
- The Editors of Encyclopaedia Britannica
Dec 17, 2021 · According to the educational website Lumen Learning, Ptolemy's complicated geocentric model stated that a planet moves in a small circle (known as an epicycle), the epicycle...
A Geocentric View. Ptolemy synthesized Greek knowledge of the known Universe. His work enabled astronomers to make accurate predictions of planetary positions and solar and lunar eclipses, promoting acceptance of his view of the cosmos in the Byzantine and Islamic worlds and throughout Europe for more than 1400 years.
Ptolemy and the Geocentric Model. Scientists of the 1500s and 1600s inherited a model of the universe whose basic features had been defined by Aristotle 2,000 years earlier. The idea was simple. Earth was stationary at the center and the Sun, Moon, and other planets all moved around Earth.
The most important solution to this problem was proposed by Claudius Ptolemy in the 3rd century AD. He argued that planets move on two sets of circles, a deferent and an epicycle. This explained retrograde motion while keeping the planets in their circular orbits around the Earth.
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