Glossary term: Heliocentric Model
Description: The term heliocentric is from the Greek helios, which is the name for the Sun, and kentro meaning center. This model of the Solar System places the Sun at the center and the planets orbit around it, replacing the geocentric (Earth-centered) model. Although the origin of the model is attributed to Copernicus in the 16th century, Aristarchus of Samos developed a heliocentric model in Ancient Greece and astronomers in India, Europe, and the Islamic world discussed such models prior to Copernicus. Observational evidence for the heliocentric model came through the telescopic observations of Venus made by Galileo. The original heliocentric model placed the Sun at the geometric center of the Solar System; this view changed with the mathematical formulations of Kepler using Tycho Brahe’s data, which Newton built on and expanded with his law of gravitation.
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Term and definition status: This term and its definition have been approved by a research astronomer and a teacher
The OAE Multilingual Glossary is a project of the IAU Office of Astronomy for Education (OAE) in collaboration with the IAU Office of Astronomy Outreach (OAO). The terms and definitions were chosen, written and reviewed by a collective effort from the OAE, the OAE Centers and Nodes, the OAE National Astronomy Education Coordinators (NAECs) and other volunteers. You can find a full list of credits here. All glossary terms and their definitions are released under a Creative Commons CC BY-4.0 license and should be credited to "IAU OAE".
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In Other Languages
- Arabic: نموذج مركزية الشمس
- Bengali: সূর্যকেন্দ্রিক মডেল
- German: Heliozentrisches Modell
- French: Modèle héliocentrique
- Italian: Modello eliocentrico
- Japanese: 地動説 (external link)
- Korean: 태양중심체계모형
- Simplified Chinese: 日心模型
- Traditional Chinese: 日心模型
Related Media
Copernicus's heliocentric system
Caption: Sketch of Copernicus's heliocentric model of the Solar System, from his book "De revolutionibus orbium coelestium" (On the revolution of the heavenly spheres) published in 1543. Shown are the Sun as well as the orbits of Mercury, Venus, the Earth (itself orbited by the Moon), Mars, Jupiter and Saturn. The outermost circle represents the sphere of the stars.
In this model, the Earth is not special – it is merely one planet, among several, orbiting the Sun. This was the first example for what is now known as the Copernican Principle: that our positions as observers in the universe is not special or privileged in any way. The shift from the geocentric to the heliocentric model of our universe is known as the Copernican revolution.
Credit: Nicolaus Copernicus
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License: PD Public Domain icons



