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Earth
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Aristotle BC 384-322
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Aristotle
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Geocentric model
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Nicolas Copernicus 1473-1543
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Eyeball observations De Revolutionibus The Earth rotates on its axis once daily and revolves around the Sun once yearly.
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Heliocentric Model
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Tycho Brahe (1546-1601)
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Johann Kepler (1571-1630)
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Kepler’s 1 st Law “ellipses”
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Kepler’s 2 nd Law “equal areas in equal times”
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PlanetPeriodDistanceP/DP/D 2 P 2 /D 3 Mercury0.240.390.621.600.99 Venus0.620.720.851.181.00 Earth1.00 Mars1.881.521.230.811.00 Jupiter11.95.202.280.441.00 Saturn29.59.513.100.331.01
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Kepler’s 3 rd Law “Harmonic Law”
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Astronomical Unit Average Distance to Sun from the Earth 1 A.U. = 150 million km Examples: Mercury 0.4 A.U. Neptune 30 A.U.
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