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The earliest-known proposal of the heliocentric model was put forward by the Greek philosopher and mathematician Aristarchus of Samos around 270 BC. He suggested that the Earth and other planets revolve around the Sun, challenging the prevailing geocentric view of the universe.
The heliocentric theory, proposed by Copernicus, states that the Sun is at the center of the solar system and that the planets, including Earth, orbit around it.
The geocentric model positioned Earth at the center of the universe with celestial bodies revolving around it. This concept was developed by ancient astronomers like Ptolemy. In contrast, the heliocentric model placed the Sun at the center with Earth and other planets orbiting around it. This idea was proposed by Nicolaus Copernicus in the 16th century and later expanded upon by Johannes Kepler and Galileo Galilei.
Heliocentric was thought to believe that the sun was at the center of the solar system and that the planets revolved around the Sun. Geocentric was thought to believe that the earth was the center of the solar system and that the planets revolved around the earth. We now know that our solar system is centered around the sun and is heliocentric.
Copernicus' heliocentric theory challenged the prevailing geocentric model of the universe, leading to a shift in scientific understanding of our place in the cosmos. This laid the foundation for modern astronomy and influenced the Scientific Revolution, sparking new ways of thinking about the universe and our place within it.
Geocentric is not a place, rather it is the name for the model of the solar system which places the earth at the centre and all other bodies revolve around it. This was considered the correct model for centuries. The heliocentric model places the sun at the centre of the solar system and all other bodies rotate around the sun. We now know this is the correct configuration.