1 / 17

Topic: Kepler’s Laws

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.

otylia
Download Presentation

Topic: Kepler’s Laws

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript

  1. Topic: Kepler’s Laws

  2. Revolution Vs. Rotation • Revolution =

  3. Revolution Vs. Rotation • Rotation =

  4. ESRT pg 15

  5. Laws of Gravity • Mass • Greater mass = • As mass increases =>

  6. Distance • The closer the objects, the stronger the gravitational forces.

  7. Modern Celestial Models • Heliocentric Model could not explain the movement of all objects, until Johannes Kepler (1609) developed laws of planetary motions

  8. 1st Law __

  9. Eccentricity A number indicating the roundness of an ellipse. Eccentricity = Distance Between Foci Length of Major Axis e=d/L Page 1 in your BEST FRIEND

  10. Perfect circle Straight line e = 1 e = 0

  11. ESRT pg 15

  12. 2nd Law __

  13. Caused by the Sun’s gravitational pull

  14. 3rd Law • __

  15. ESRT pg 15

  16. Final Question • http://www.polleverywhere.com/multiple_choice_polls/OTk2MDQ2MzY2/web

More Related