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  2. Geocentric model - Wikipedia

    en.wikipedia.org/wiki/Geocentric_model

    The Earth and Moon are much closer to being a binary planet; the center of mass around which they both rotate is still inside the Earth, but is about 4,624 km (2,873 miles) or 72.6% of the Earth's radius away from the centre of the Earth (thus closer to the surface than the center).

  3. Deferent and epicycle - Wikipedia

    en.wikipedia.org/wiki/Deferent_and_epicycle

    The angular rate at which the epicycle traveled was not constant unless he measured it from another point which is now called the equant (Ptolemy did not give it a name). It was the angular rate at which the deferent moved around the point midway between the equant and the Earth (the eccentric) that was constant; the epicycle center swept out ...

  4. Ptolemaic Kingdom - Wikipedia

    en.wikipedia.org/wiki/Ptolemaic_Kingdom

    Ptolemy as Pharaoh of Egypt, British Museum, London. In 332 BC, Alexander the Great, King of Macedon, conquered Egypt, which at the time was a satrapy of the Achaemenid Empire later called Egypt's Thirty-first Dynasty. [16] He visited Memphis, and travelled to the oracle of Amun at the Siwa Oasis. The oracle declared him to be the son of Amun.

  5. De revolutionibus orbium coelestium - Wikipedia

    en.wikipedia.org/wiki/De_revolutionibus_orbium...

    The world (heavens) is spherical, as is the Earth, and the land and water make a single globe. The celestial bodies, including the Earth, have regular circular and everlasting movements. The Earth rotates on its axis and around the Sun. [5] Answers to why the ancients thought the Earth was central. The order of the planets around the Sun and ...

  6. Ptolemy's world map - Wikipedia

    en.wikipedia.org/wiki/Ptolemy's_world_map

    The Ptolemy world map is a map of the world known to Greco-Roman societies in the 2nd century. It is based on the description contained in Ptolemy 's book Geography , written c. 150 . Based on an inscription in several of the earliest surviving manuscripts, it is traditionally credited to Agathodaemon of Alexandria .

  7. Copernican Revolution - Wikipedia

    en.wikipedia.org/wiki/Copernican_Revolution

    Nicolaus Copernicus's heliocentric model. Copernicus studied at Bologna University during 1496–1501, where he became the assistant of Domenico Maria Novara da Ferrara.He is known to have studied the Epitome in Almagestum Ptolemei by Peuerbach and Regiomontanus (printed in Venice in 1496) and to have performed observations of lunar motions on 9 March 1497.

  8. The time when a day on Earth was just 19 hours long - AOL

    www.aol.com/lifestyle/day-earth-used-just-19...

    Known affectionately to scientists as the "boring billion," there was a seemingly endless period in the world's history when the length of a day stayed put.

  9. Ancient Greek astronomy - Wikipedia

    en.wikipedia.org/wiki/Ancient_Greek_astronomy

    Bounded elongation is the angular distance of celestial bodies from the center of the universe. Ptolemy's model of the cosmos and his studies landed him an important place in history in the development of modern-day science. In the Ptolemaic system, the Earth was at the center of the universe with the Moon, the Sun, and five planets circling it.