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22.1 Early Astronomy.

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Presentation on theme: "22.1 Early Astronomy."— Presentation transcript:

1 22.1 Early Astronomy

2 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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4 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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6 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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8 Watch retrograde motion!
BBC Video

9 The path a planet follows around the sun is called its orbit

10 Kepler’s Laws of Planetary Motion
1st law : planets orbit the sun in a path called an ellipse

11 perihelion aphelion

12 astronomical unit: the average distance between the earth and the sun
150 million km 93 million miles

13 2nd law: planets move fastest when they are closest to the sun in their orbits

14 3rd law: the farther away a planet orbits, the longer the planet takes to revolve around the sun


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