The Copernican RevolutionPage
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Kepler’s third law can be derived from Newton’s law of gravity
F = GMm/r2 = mg
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Gravity
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Contents
- The Copernican Revolution
- What do we see in the sky?
- Timeline
- Geocentric (Ptolemaic) System
- Heliocentric (Copernican) System
- Geocentric vs. Heliocentric
- Phases of Venus
- Geocentric vs. Heliocentric
- Stellar Parallax
- Copernicus vs. the Church
- Misconceptions
- Galileo Galilei
- Tycho Brahe
- Tycho Brahe
- The skies change
- A new star
- Comet of 1577
- Johannes Kepler
- Mathematical perfection
- The battle with Mars
- Astronomia nova
- Kepler’s first Law
- Kepler’s second law
- Kepler’s Third Law
- Other Solar System Bodies
- A force for planetary motion
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