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Ptolemaic system

American  

noun

Astronomy.
  1. a system elaborated by Ptolemy and subsequently modified by others, according to which the earth was the fixed center of the universe, with the heavenly bodies moving about it.


Ptolemaic system British  

noun

  1. the theory of planetary motion developed by Ptolemy from the hypotheses of earlier philosophers, stating that the earth lay at the centre of the universe with the sun, the moon, and the known planets revolving around it in complicated orbits. Beyond the largest of these orbits lay a sphere of fixed stars See also epicycle Compare Copernican system

"Collins English Dictionary — Complete & Unabridged" 2012 Digital Edition © William Collins Sons & Co. Ltd. 1979, 1986 © HarperCollins Publishers 1998, 2000, 2003, 2005, 2006, 2007, 2009, 2012

Ptolemaic system Scientific  
/ tŏl′ə-māĭk /
  1. The astronomical system of Ptolemy, in which Earth is at the center of the universe and all celestial bodies revolve around it. The Sun, Moon, and planets revolve at different levels in circular orbits, and the stars lie in fixed locations on a sphere that revolves beyond these orbits.

  2. See more at epicycle


Etymology

Origin of Ptolemaic system

First recorded in 1765–75

Example Sentences

Examples are provided to illustrate real-world usage of words in context. Any opinions expressed do not reflect the views of Dictionary.com.

Though Copernicus’s system didn’t agree with the data completely—the circular orbits were wrong, though the heliocentric idea was correct—it was much simpler than the Ptolemaic system.

From Literature

The thing that most worried him about the Ptolemaic system, typified by the puzzle of the Moon, was the business of equants.

From Literature

Part of his purpose was to prove that the Ptolemaic system was an accurate representation of how the heavens really work and not just a mathematical model.

From Literature

For a thousand years the Ptolemaic system was believed all round the world.

From The Guardian

The Ptolemaic system was too strongly intrenched, and the motions of all the bodies in the sky were too well represented by it.

From Project Gutenberg