The historical models of our solar system, from oldest to most recent, would be as follows:
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Geocentric Model (Ancient Greece) - This model, primarily associated with Claudius Ptolemy, placed the Earth at the center of the universe, with all other celestial bodies orbiting around it.
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Heliocentric Model (16th Century) - Proposed by Nicolaus Copernicus, this model suggested that the Sun is at the center of our solar system, with the Earth and other planets orbiting around it.
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Kepler's Laws of Planetary Motion (early 17th Century) - Johannes Kepler developed three laws that described the motion of planets around the Sun, introducing the idea of elliptical orbits rather than circular ones.
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Newton's Law of Universal Gravitation (1687) - Isaac Newton's work further explained planetary motion through the concept of gravity, solidifying the heliocentric model and providing the mathematical framework for planetary orbits.
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Modern Solar System Model (20th Century to Present) - This includes discoveries related to the composition of planets, the recognition of the role of gravity at a larger scale, the understanding of the solar system's formation, and the existence of exoplanets.
In summary, the accurate order is:
- Geocentric Model
- Heliocentric Model
- Kepler's Laws of Planetary Motion
- Newton's Law of Universal Gravitation
- Modern Solar System Model