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  2. Deferent and epicycle - Wikipedia

    en.wikipedia.org/wiki/Deferent_and_epicycle

    Apollonius of Perga (3rd century BC) realized that this cyclical variation could be represented visually by small circular orbits, or epicycles, revolving on larger circular orbits, or deferents. Hipparchus (2nd century BC) calculated the required orbits. Deferents and epicycles in the ancient models did not represent orbits in the modern sense ...

  3. Newton's theorem of revolving orbits - Wikipedia

    en.wikipedia.org/wiki/Newton's_theorem_of...

    To describe this forward-and-backward motion, Apollonius of Perga (c. 262 – c. 190 BC) developed the concept of deferents and epicycles, according to which the planets are carried on rotating circles that are themselves carried on other rotating circles, and so on.

  4. Equant - Wikipedia

    en.wikipedia.org/wiki/Equant

    Applied without an epicycle (as for the Sun), using an equant allows for the angular speed to be correct at perigee and apogee, with a ratio of (+) / (where is the orbital eccentricity). But compared with the Keplerian orbit , the equant method causes the body to spend too little time far from the Earth and too much close to the Earth.

  5. Commentariolus - Wikipedia

    en.wikipedia.org/wiki/Commentariolus

    For the ratios of the radii of the outer planets' deferents to radius of the Earth, the Commentariolus gives 1 13 ⁄ 25 for Mars, 5 13 ⁄ 60 for Jupiter, and 9 7 ⁄ 30 for Saturn. For the ratios of the radii of their deferents to the radii of the larger of their epicycles, it gives 6 138 ⁄ 167 for Mars, 12 553 ⁄ 606 for Jupiter, and 11 ...

  6. Lewy's example - Wikipedia

    en.wikipedia.org/wiki/Lewy's_example

    In the mathematical study of partial differential equations, Lewy's example is a celebrated example, due to Hans Lewy, of a linear partial differential equation with no solutions. It shows that the analog of the Cauchy–Kovalevskaya theorem does not hold in the smooth category.

  7. De revolutionibus orbium coelestium - Wikipedia

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

    Book III describes his work on the precession of the equinoxes and treats the apparent movements of the Sun and related phenomena. Book IV is a similar description of the Moon and its orbital movements. Book V explains how to calculate the positions of the wandering stars based on the heliocentric model and gives tables for the five planets.

  8. Geocentric model - Wikipedia

    en.wikipedia.org/wiki/Geocentric_model

    Size of deferents, epicycles Only ratio between radius of deferent and associated epicycle determined; absolute distances not determined in theory Interior planets: Average greatest elongations of 23° (Mercury) and 46° (Venus) Size of epicycles set by these angles, proportional to distances Interior planets Limited to movement near the Sun

  9. Apparent retrograde motion - Wikipedia

    en.wikipedia.org/wiki/Apparent_retrograde_motion

    In the geocentric model of the Solar System proposed by Apollonius in the third century BCE, retrograde motion was explained by having the planets travel in deferents and epicycles. [4] It was not understood to be an illusion until the time of Copernicus , although the Greek astronomer Aristarchus in 240 BCE proposed a heliocentric model for ...