Geocentrism
Geocentrism is an astronomical model positing that Earth is stationary at the center of the universe, with the Sun, Moon, planets, and stars orbiting it in various paths.[1] Originating in ancient Greek cosmology around 380 BCE with Eudoxus's system of concentric spheres, it was refined by Aristotle and later formalized by Claudius Ptolemy in the 2nd century CE through the introduction of epicycles and deferents to account for observed planetary retrogrades.[1][2] This Ptolemaic system dominated Western and Islamic astronomy for over a millennium, providing predictive accuracy for celestial positions sufficient for calendars and navigation despite its mathematical complexity.[3][4] Empirical observations, including Galileo's telescopic discovery of Jupiter's moons in 1610, the phases of Venus consistent with heliocentric orbits, stellar aberration by James Bradley in 1727, and the measurement of stellar parallax in 1838, progressively falsified the model's core assumption of an immobile Earth.[5][6] Modern evidence from space probes, such as Voyager missions revealing planetary systems beyond simple geocentric kinematics, and Earth's rotation demonstrated by the Foucault pendulum and Coriolis effects, confirms heliocentrism and broader relativistic frameworks over any absolute geocentrism.[6] While historically influential, geocentrism lacks support in contemporary physics, with fringe modern advocates often relying on reinterpretations of relativity rather than direct empirical validation.[7]