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Renaissance Astronomy
Chapter 4
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The Universe as described in Dante’s Divine Comedy
Fig. 4.1 The Universe as described in Dante’s Divine Comedy
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Timeline and Notable People and Events (Left)
Fig. 4.2 Timeline and Notable People and Events (Left) And Four Most Prominent Renaissance Astronomers (Copernicus, Tycho, Kepler, Galileo)
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Copernicus
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Heliocentric Model (Copernicus)
Fig. 4.3 Heliocentric Model (Copernicus)
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Retrograde motion according to the heliocentric model
Fig. 4.4 Retrograde motion according to the heliocentric model
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Fig. 4.5
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Fig. 4.6
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Fig. 4.6 Greatest Elongation
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Mars’ epicycle in Copernicus’ model
Fig. 4.7 Mars’ epicycle in Copernicus’ model
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Fig. 4.8
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Tycho Brahe
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Fig. 4.9 Tycho Brahe
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Fig. 4.10 Parallax of a Star Distance = 1/parallax
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Kepler
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Fig. 4.12 Ellipses
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Kepler’s first law: Planets move around the Sun in ellipses
Fig. 4.13 Kepler’s first law: Planets move around the Sun in ellipses
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Kepler’s second law: Planets sweeps out equal areas at equal times
Fig. 4.14 Kepler’s second law: Planets sweeps out equal areas at equal times
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Kepler’s 3rd law Kepler’s third law
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Galileo
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Fig. 4.15 Galileo’s Drawings of the moon
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Fig. 4.16
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Fig. 4.17
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