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EARTH SCIENCE MRS. DAVIS

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Presentation on theme: "EARTH SCIENCE MRS. DAVIS"— Presentation transcript:

1 EARTH SCIENCE MRS. DAVIS
The Universe EARTH SCIENCE MRS. DAVIS

2 Our View of the Cosmos Astronomy has seen 3 scientific revolutions in cosmology… 2nd Century: Claudius Ptolemy (Physics of Aristotle) Geocentric: Earth-centered model of the universe 16th Century: Nicolaus Copernicus (Physics of Newton) Heliocentric: Sun-centered model of the universe 20th Century: Edwin Hubble (Physics of Einstein) Big Bang Cosmology

3 Geocentric Model

4 What’s wrong with this idea?
The geocentric model couldn’t explain retrograde motion. Planets like Mars look like they drift from side to side.

5 Retrograde Motion

6 Heliocentric Model

7 New(ish) Ideas -- Brahe
Didn’t believe the heliocentric model Stars should demonstrate parallax Apparent shift in position

8 New(ish) Ideas -- Kepler
Developed 3 laws of planetary motion

9 Kepler’s 1st Law Orbits are shaped like an ellipse with sun as one focus Perihelion-closest to the sun Aphelion- farthest from the sun Major Axis Minor (semi-major) axis Keplers 1st Law

10 Ellipse

11 Ellipse

12 Kepler’s 2nd Law A planet sweeps out an equal area in equal time no matter how fast it is moving.

13 Kepler’s 2nd Law

14 Kepler’s 3rd Law The farther away a planet is from the sun, the longer it takes for one complete period. 1 astronomical unit (1 AU) is the average distance from sun to Earth

15 New(ish) Ideas -- Galileo
Created telescope Observed Jupiter’s moons Saw planets are spheres Moon surface Sun spots House arrest

16 New(ish) Ideas -- Newton
Law of Universal Gravitation: Gravity keeps planets from flying away Mass is proportional (Mass goes up, gravitational force goes up) Longer the radius, weaker the gravitational pull.


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