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  2. Phases of Venus - Wikipedia

    en.wikipedia.org/wiki/Phases_of_Venus

    The first observations of the full planetary phases of Venus were by Galileo at the end of 1610 (though not published until 1613 in the Letters on Sunspots).Using a telescope, Galileo was able to observe Venus going through a full set of phases, something prohibited by the Ptolemaic system that assumed Venus to be a perfect celestial body.

  3. Geocentric model - Wikipedia

    en.wikipedia.org/wiki/Geocentric_model

    The geocentric model held sway into the early modern age, but from the late 16th century onward, it was gradually superseded by the heliocentric model of Copernicus (1473–1543), Galileo (1564–1642), and Kepler (1571–1630). There was much resistance to the transition between these two theories, since for a long time the geocentric ...

  4. File:Phases-of-Venus2.svg - Wikipedia

    en.wikipedia.org/wiki/File:Phases-of-Venus2.svg

    In contrast, the geocentric model of Ptolemy predicted that only crescent and new phases would be seen, since Venus was thought to remain between the Sun and Earth during its orbit around the Earth. Galileo's observations of the phases of Venus proved that it orbited the Sun and lent support to (but did not prove) the heliocentric model. Source

  5. Tychonic system - Wikipedia

    en.wikipedia.org/wiki/Tychonic_system

    It is conceptually a geocentric model, ... The Tychonic system was an acceptable alternative as it explained the observed phases of Venus with a static Earth.

  6. File:Phases-of-Venus-Geocentric.svg - Wikipedia

    en.wikipedia.org/wiki/File:Phases-of-Venus...

    In the geocentric model of the solar system, as Venus moves on its epicycle (while the epicycle moves around the Earth), it is always in between the Earth and the Sun. Therefore, the only possible phases of Venus would be new and crescent phases.

  7. Copernican Revolution - Wikipedia

    en.wikipedia.org/wiki/Copernican_Revolution

    In 1610, Galileo observed that Venus had a full set of phases, similar to the phases of the moon we can observe from Earth. This was explainable by the Copernican or Tychonic systems which said that all phases of Venus would be visible due to the nature of its orbit around the Sun, unlike the Ptolemaic system which stated only some of Venus's ...

  8. Historical models of the Solar System - Wikipedia

    en.wikipedia.org/wiki/Historical_models_of_the...

    Around 420 AD Martianus Capella describes a modified geocentric model, in which the Earth is at rest in the center of the universe and circled by the Moon, the Sun, three planets and the stars, while Mercury and Venus circle the Sun. [50] His model was not widely accepted, despite his authority; he was one of the earliest developers of the ...

  9. Paul Wittich - Wikipedia

    en.wikipedia.org/wiki/Paul_Wittich

    Renowned anti-Copernican adherents of the Capellan planetary model included Francis Bacon, inter alia, and this model appealed to those who accepted Ptolemy's purely geocentric model was refuted by the phases of Venus, but were unpersuaded by Tychonic arguments that Mars, Jupiter and Saturn also orbited the Sun in addition to Mercury and Venus ...