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22.1 Early Astronomy
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Solar System Models geocentric model: model of the solar system that states that the Earth is the center of the solar system believed until 1600’s
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heliocentric model: model of the solar system that states that the sun is the center of the solar system and the planets revolve around it
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the stars don’t seem to move in our sky; planets do because they are much closer than stars
planets move in an eastward movement sometimes planets appear to move in a backward movement, this is called retrograde motion a loop occurs because each planet travels around the sun at different speeds
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Watch retrograde motion!
BBC Video
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The path a planet follows around the sun is called its orbit
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Kepler’s Laws of Planetary Motion
1st law : planets orbit the sun in a path called an ellipse
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perihelion aphelion
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astronomical unit: the average distance between the earth and the sun
150 million km 93 million miles
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2nd law: planets move fastest when they are closest to the sun in their orbits
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3rd law: the farther away a planet orbits, the longer the planet takes to revolve around the sun
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