Copernicus
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The sun-centered theory, known as heliocentrism, was confirmed by observations made by the Polish astronomer Nicolaus Copernicus in the 16th century and further supported by the observations of Galileo Galilei in the 17th century. The idea that the Earth revolves around the sun replaced the previously widely accepted geocentric model.
Galileo.
The heliocentric, or Sun-centered, system was first theorized by Nicolaus Copernicus.
The sun-centered model, or heliocentric model, is the scientific theory that places the sun at the center of the solar system, with the planets orbiting around it. This model, proposed by Copernicus in the 16th century, replaced the Earth-centered model (geocentric model) that had been widely accepted. Today, the heliocentric model is the basis for our understanding of the structure of the solar system.
The heliocentric theory was originated by Copernicus.
Both the Copernican and Ptolemaic models were geocentric theories that sought to explain the motion of celestial bodies, particularly the movement of the Sun, Moon, and planets in relation to Earth. However, the key difference between the two theories lies in their proposed structure of the solar system, with Copernicus advocating a heliocentric model (Sun-centered) while Ptolemy supported a geocentric model (Earth-centered).