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Earth Aristotle BC 384-322 Aristotle Geocentric model.

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Presentation on theme: "Earth Aristotle BC 384-322 Aristotle Geocentric model."— Presentation transcript:

1

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3 Earth

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5 Aristotle BC 384-322

6 Aristotle

7 Geocentric model

8 Nicolas Copernicus 1473-1543

9 Eyeball observations De Revolutionibus The Earth rotates on its axis once daily and revolves around the Sun once yearly.

10 Heliocentric Model

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12 Tycho Brahe (1546-1601)

13 Johann Kepler (1571-1630)

14 Kepler’s 1 st Law “ellipses”

15 Kepler’s 2 nd Law “equal areas in equal times”

16 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

17 Kepler’s 3 rd Law “Harmonic Law”

18 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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