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Copernican Theory

The Copernican theory, also known as the Heliocentric model, was a revolutionary astronomical model developed by Nicolaus Copernicus in the 16th century. This theory posits that:

Historical Context

Before Copernicus, the predominant cosmological model was the Ptolemaic system or Geocentric model, which placed Earth at the center of the universe with all celestial bodies, including the Sun, orbiting around it. This model was largely accepted due to the apparent movement of the stars and planets across the sky, which seemed to support Earth's immobility.

Copernicus, influenced by earlier heliocentric ideas from Aristarchus of Samos and others, began to develop his theory in the early 1500s. His work, "De revolutionibus orbium coelestium" (On the Revolutions of the Heavenly Spheres), was published in 1543, the year of his death. In this seminal work, Copernicus presented a detailed mathematical model of a heliocentric system:

Implications and Reception

The Copernican theory was initially met with resistance:

However, the model gradually gained acceptance, especially after:

The acceptance of the Copernican theory was a pivotal moment in the Scientific Revolution, contributing to:

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