Presentation is loading. Please wait.

Presentation is loading. Please wait.

Kepler’s Laws of Planetary Motion

Similar presentations


Presentation on theme: "Kepler’s Laws of Planetary Motion"— Presentation transcript:

1 Kepler’s Laws of Planetary Motion
The Law of Ellipses The Law of Equal Area The Law of Harmonies

2 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.

3 Planets travel the same amount of area in the same amount of time in their orbits.
The Law of Equal Area

4

5 The rate of revolution depends on distance from the sun.
The Law of Harmonies The rate of revolution depends on distance from the sun.

6 How do celestial objects stay in orbit?

7 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*

8 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.

9

10 Use Your ESRT p. 1

11 Eccentricity Eccentricity is measured on a scale of 0-1
The farther apart the foci, the higher the eccentricity

12 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

13 Length of Major Axis- 15cm Distance between Foci-5cm
Example Problem Length of Major Axis- 15cm Distance between Foci-5cm

14 Length of Major Axis- 17cm Distance between Foci- 7cm
Example Problem Length of Major Axis- 17cm Distance between Foci- 7cm

15 Use Your ESRT p. 15

16 What is a planet’s favorite gum?
Orbit


Download ppt "Kepler’s Laws of Planetary Motion"

Similar presentations


Ads by Google