kepler’s laws

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Kepler’s Laws

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Kepler’s Laws. Kepler’s Laws. Johannes Kepler Mars’ orbit is not a perfect circle, it is elliptical The speed of Mars’ orbit changes Closer to sun = faster Farther away from sun = slower Lead to Kepler’s 3 Laws. Kepler’s 1 st Law. - PowerPoint PPT Presentation

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Page 1: Kepler’s  Laws

Kepler’s Laws

Page 2: Kepler’s  Laws

Kepler’s LawsJohannes Kepler

Mars’ orbit is not a perfect circle, it is elliptical

The speed of Mars’ orbit changes

Closer to sun = faster

Farther away from sun = slower

Lead to Kepler’s 3 Laws

Page 3: Kepler’s  Laws

Kepler’s 1st LawThe path of each planet around the sun is an ellipse with the sun at one focus

Page 4: Kepler’s  Laws

Kepler’s 2nd LawEach planet revolves so that the “imaginary line” that connects it to the sun sweeps equal amount of area in equal time intervals

Closer to sun = faster

Farther away = slower

Page 5: Kepler’s  Laws

Kepler’s 3rd LawThe square of a planet’s orbital period is proportional to the cube of its distance from the sun

Orbital period - how long it takes to orbit the sun

Astronomical Unit (AU) – average distance between Earth and sun – 150 million km

T2 = d3 ; T = orbital period, d=distance from sun in AUs

Page 6: Kepler’s  Laws

Kepler’s 3rd LawT2 = d3

Mars has period (T) of 1.88 years (T = 1.88)

(1.88)2 = 3.54

d3 = 3.54

d = 1.52 AU

Page 7: Kepler’s  Laws

Kepler’s Laws Tri-fold

Use a tri-fold/brochure to explain Kepler’s 3 Laws. There should be no words other than labeling each 3rd as to which law you are demonstrating. You may also use the formula for Kepler’s 3rd law.

Page 8: Kepler’s  Laws

OrbitsBarycenter – point between two objects where they balance each other

When a moon orbits planet, or planet orbits a star, both bodies are orbiting around a point that lies outside of the larger body (star/planet)

http://en.wikipedia.org/wiki/Barycentric_coordinates_(astronomy)

http://www.youtube.com/watch?v=KnHUAc20WEU

http://www.youtube.com/watch?v=rKo6tfFtZg8(2:59)

Page 9: Kepler’s  Laws

OrbitsThe Sun is NOT a stationary object.

Sun moves as the planets tug on it

Sun orbits the solar system’s barycenter

Page 10: Kepler’s  Laws

Moon and Earth Relationship

Earth pulls on the moon, and moon pulls on Earth

This “tugging” from the moon can cause the Earth to bulge

Page 11: Kepler’s  Laws

Moon and Earth Relationship

Earth’s solids cannot give, however water does, causing our tides

Two high tides and two low tides a day

12hrs and 25 min between two high tides

Page 12: Kepler’s  Laws

Moon and Earth Relationship

Rise and fall daily due to Earth, Sun, and Moon interactions

Since earth is rotating, we experience two tides each day

Page 13: Kepler’s  Laws

Moon and Earth Relationship

Spring Tides – when moon and sun interact together and form extreme tides.

Occurs during full and new moons

Page 14: Kepler’s  Laws

Moon and Earth Relationship

Neap Tides – moon and sun pull at right angles and cancel each other out...very weak tides

http://www.youtube.com/watch?v=l37ofe9haMU

http://www.youtube.com/watch?v=rRPtNAA-9UE