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Kepler’s Laws of Planetary Motion
The Law of Ellipses The Law of Equal Area The Law of Harmonies
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Planets travel in an elliptical orbit with one focus being the sun.
The Law of Ellipses Planets travel in an elliptical orbit with one focus being the sun.
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Planets travel the same amount of area in the same amount of time in their orbits.
The Law of Equal Area
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The rate of revolution depends on distance from the sun.
The Law of Harmonies The rate of revolution depends on distance from the sun.
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How do celestial objects stay in orbit?
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Inertia An object in motion tends to stay in motion An object at rest
tends to stay at rest *unless acted upon by an outside force*
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Gravity The force of gravity decreases with distance from center of gravity. When a planet is farthest from the sun there is less of a gravitational pull. This causes a planet to move slowest in it’s orbit when farthest from the sun.
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Use Your ESRT p. 1
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Eccentricity Eccentricity is measured on a scale of 0-1
The farther apart the foci, the higher the eccentricity
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Eccentricity- How elongated an ellipse is
Ellipse- A shape drawn using two foci Focus- A point on the major axis used to draw an ellipse (Plural-Foci) Major Axis- The longest line that goes through the center of the ellipse
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Length of Major Axis- 15cm Distance between Foci-5cm
Example Problem Length of Major Axis- 15cm Distance between Foci-5cm
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Length of Major Axis- 17cm Distance between Foci- 7cm
Example Problem Length of Major Axis- 17cm Distance between Foci- 7cm
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Use Your ESRT p. 15
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What is a planet’s favorite gum?
Orbit
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