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Topic: Kepler’s Laws

Topic: Kepler’s Laws

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Topic: Kepler’s Laws. Revolution Vs. Rotation. Revolution =. Revolution Vs. Rotation. Rotation =. ESRT pg 15. Laws of Gravity. Mass Greater mass = As mass increases =>. Distance The closer the objects, the stronger the gravitational forces. Modern Celestial Models. - PowerPoint PPT Presentation

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Page 1: Topic:   Kepler’s  Laws

Topic: Kepler’s Laws

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Revolution Vs. Rotation

• Revolution =

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Revolution Vs. Rotation

• Rotation =

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ESRT pg 15

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Laws of Gravity

• Mass – Greater mass =– As mass increases =>

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• Distance – The closer the objects, the stronger the

gravitational forces.

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Modern Celestial Models• Heliocentric Model could

not explain the movement of all objects, until Johannes Kepler (1609) developed laws of planetary motions

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1st Law __

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EccentricityA number indicating the roundness of

an ellipse.

Eccentricity = Distance Between Foci

Length of Major Axis

e=d/L Page 1 in your BEST FRIEND

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e = 0 e = 1

Perfect circle

Straight line

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ESRT pg 15

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2nd Law__

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Caused by the Sun’s gravitational pull

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3rd Law• __

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ESRT pg 15

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Final Question

• http://www.polleverywhere.com/multiple_choice_polls/OTk2MDQ2MzY2/web