Epicycle 2026-11-05
An epicycle is a circle whose centre moves along another path, traditionally a larger circle called the deferent. Combining these motions can reproduce loops and changes of apparent speed in a planet's position on the celestial sphere. In Ptolemy's geocentric model, such constructions supplied quantitative planetary predictions.[ref]
A simple planar example is
The second term is the epicycle relative to its moving centre. Suitable radii and angular rates can produce locally backward motion, illustrating apparent retrograde motion. The construction is a geometric representation; fitting an observed track does not by itself establish what force governs the actual orbit.
Ptolemy Created 2026-10-24 Updated 2026-11-05
Ptolemy developed a mathematical system for predicting celestial motion in the Almagest by Ptolemy. The work combines a stationary central Earth with geometrical models and observational parameters for the apparent paths of the Sun, Moon and planets.
An epicycle is a circle whose center travels on another circle. Adding these motions can produce an apparent backward loop even though the component rotations continue steadily. This illustrates the predictive purpose of the construction: observed angular behavior is represented by organized component motions. A successful fit of sky directions does not by itself uniquely establish the physical arrangement of the bodies.[ref]
Figure 1.
Portrait of Ptolemy
. Unknown engraver, in André Thevet, Les vrais portraits et vies des hommes illustres (1584), folio 87; scan via UQAM. Public domain (PD-Art, life+100/pre-1931 publication). Source and usage information on the linked Wikimedia file page. Source.