How did Nicolaus Copernicus describe Earth’s yearly motion?

Created from Britannica articles using AI. AI can make mistakes, so verify using Britannica articles.

Nicolaus Copernicus proposed that Earth is a planet that orbits the Sun annually. In his heliocentric system, he described the Sun as the fixed point to which the motions of the planets are referred, effectively setting Earth into motion around it.12

Copernicus concluded that the observed planetary motions—such as the retrograde motion of superior planets—were not independent phenomena but were instead manifestations of Earth’s own motion as it travels in its yearly orbit. This model was detailed in his seminal work, De revolutionibus orbium coelestium libri VI, published in 1543.31