heliosentrisessä
Heliocentrisessä, or the heliocentric model, is a scientific paradigm that places the Sun at the center of the solar system, with the planets, including Earth, revolving around it in defined orbits. This concept fundamentally contrasts with the geocentric model, which historically positioned Earth as the immovable center of the universe. The heliocentric theory was first proposed by the ancient Greek astronomer Aristarchus of Samos around 250 BCE, though it gained broader acceptance only after the work of Nicolaus Copernicus in the 16th century. Copernicus’s *De Revolutionibus Orbium Coelestium* (On the Revolutions of the Heavenly Spheres) systematically argued for a Sun-centered solar system, challenging the long-held geocentric views of Ptolemy and the Catholic Church.
The heliocentric model was later refined by Johannes Kepler, who formulated his three laws of planetary motion
Today, the heliocentric model is universally accepted as the correct description of the solar system’s structure.