Earth Aristotle BC 384-322 Aristotle Geocentric model.

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Presentation transcript:

Earth

Aristotle BC

Aristotle

Geocentric model

Nicolas Copernicus

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

Heliocentric Model

Tycho Brahe ( )

Johann Kepler ( )

Kepler’s 1 st Law “ellipses”

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

PlanetPeriodDistanceP/DP/D 2 P 2 /D 3 Mercury Venus Earth1.00 Mars Jupiter Saturn

Kepler’s 3 rd Law “Harmonic Law”

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.