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Copernican heliocentrism is the astronomical model developed by the Renaissance astronomer Nicolaus Copernicus and published in 1543. This model positioned the Sun near the center of the Universe, motionless, with Earth and the other planets orbiting around it in circular paths, modified by epicycles, and at uniform speeds. The Copernican model…
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| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| Copernican heliocentrism | is a | astronomical model developed by the Renaissance astronomer Nicolaus Copernicus and published in 1543 | 0.90 | text |
| the planets' circular orbits | instance of | His heliostatic model retained several false Ptolemaic assumptions | 0.80 | text |
| epicycles | instance of | His heliostatic model retained several false Ptolemaic assumptions | 0.80 | text |
| and uniform speeds | instance of | His heliostatic model retained several false Ptolemaic assumptions | 0.80 | text |
| while at the same time using accurate ideas such as | instance of | His heliostatic model retained several false Ptolemaic assumptions | 0.80 | text |
| eccentrics | instance of | Also popular with astronomers were variations | 0.80 | text |
| Galileo | instance of | Copernicus' model did have a large influence on later scientists | 0.80 | text |
| Johannes Kepler | instance of | Copernicus' model did have a large influence on later scientists | 0.80 | text |
| who adopted | instance of | Copernicus' model did have a large influence on later scientists | 0.80 | text |
| championed and | instance of | Copernicus' model did have a large influence on later scientists | 0.80 | text |
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