Copernicus Publishes Heliocentric Model

On the day of his death (24 May 1543), Nicolaus Copernicus received the first printed copy of De revolutionibus orbium coelestium — 'On the Revolutions of the Celestial Spheres.' The book argued that the Sun, not the Earth, sits at the centre of the solar system, and that the Earth orbits the Sun annually while rotating on its own axis daily. This overturned the Ptolemaic geocentric model that had dominated European astronomy for 1,400 years and aligned with Church teaching. Copernicus was cautious: he dedicated the book to Pope Paul III and framed his model as a mathematical convenience. The book was not immediately condemned — that came later when Galileo made the model publicly popular and confrontational. The Copernican Revolution required three generations to complete: Tycho Brahe (1546–1601) refined observational data; Johannes Kepler (1571–1630) derived the elliptical laws of planetary motion; Galileo (1564–1642) provided telescopic evidence; Newton (1643–1727) explained the force (gravity) that makes the system work. Together they represent the founding of modern science — the replacement of authority and tradition by observation, mathematics, and falsifiable theory.

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