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  2. Geocentric model - Wikipedia

    en.wikipedia.org/wiki/Geocentric_model

    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the geocentric model (also known as geocentrism, often exemplified specifically by the Ptolemaic system) is a superseded description of the Universe with Earth at the center.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.

  3. Deferent and epicycle - Wikipedia

    en.wikipedia.org/wiki/Deferent_and_epicycle

    In the Hipparchian, Ptolemaic, and Copernican systems of astronomy, the epicycle (from Ancient Greek ἐπίκυκλος (epíkuklos) 'upon the circle', meaning "circle moving on another circle") [1] was a geometric model used to explain the variations in speed and direction of the apparent motion of the Moon, Sun, and planets.

  4. List of topics characterized as pseudoscience - Wikipedia

    en.wikipedia.org/wiki/List_of_topics...

    Modern geocentrism – In astronomy, the geocentric model (also known as geocentrism or the Ptolemaic system) is a superseded description of the universe with Earth at the center. Under the geocentric model, the Sun, Moon, stars and planets all circled Earth.

  5. Equant - Wikipedia

    en.wikipedia.org/wiki/Equant

    The basic elements of Ptolemaic astronomy, showing a planet on an epicycle (smaller dashed circle), a deferent (larger dashed circle), the eccentric (×) and an equant (•). Equant (or punctum aequans) is a mathematical concept developed by Claudius Ptolemy in the 2nd century AD to account for the observed motion of the planets. The equant is ...

  6. Primum Mobile - Wikipedia

    en.wikipedia.org/wiki/Primum_Mobile

    In classical, medieval, and Renaissance astronomy, the Primum Mobile (Latin: "first movable") was the outermost moving sphere in the geocentric model of the universe. [ 1 ] The concept was introduced by Ptolemy to account for the apparent daily motion of the heavens around the Earth, producing the east-to-west rising and setting of the sun and ...

  7. Celestial spheres - Wikipedia

    en.wikipedia.org/wiki/Celestial_spheres

    Ptolemaic model of the spheres for Venus, Mars, Jupiter, and Saturn with epicycle, eccentric deferent and equant point. Georg von Peuerbach , Theoricae novae planetarum , 1474. In his Almagest , the astronomer Ptolemy (fl. c. 150 AD) developed geometrical predictive models of the motions of the stars and planets and extended them to a unified ...

  8. Ptolemaic - Wikipedia

    en.wikipedia.org/wiki/Ptolemaic

    Ptolemaic is the adjective formed from the name Ptolemy, ... Ptolemaic system, a geocentric model of the universe developed in detail by the astronomer Claudius ...

  9. The Discarded Image - Wikipedia

    en.wikipedia.org/wiki/The_Discarded_Image

    It was his last book and deals with medieval cosmology and the Ptolemaic universe. It portrays the medieval conception of a "model" of the world, which Lewis described as "the medieval synthesis itself, the whole organization of their theology, science and history into a single, complex, harmonious mental model of the universe." [1]