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Astronomy 171
Solar System Astronomy
Prof. Paul Martini
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Lecture 14: Brahe and Kepler
Key Ideas
- Tycho Brahe
- Amassed 20 years of precise planetary data
- Johannes Kepler
- Brilliant theorist who analyzed Tycho's data
- Kepler's Three Laws of Planetary Motion
- 1st Law: Orbits are Ellipses with Sun at 1 focus
- 2nd Law: Equal Areas Law
- 3rd Law: (Period)2 = (Semi-major Axis)3
Tycho Brahe (1546 - 1601)
- Danish nobleman, brilliant astronomer, and instrument builder
- Admired Copernicus as a mathematician
- Did not like the idea of a moving Earth
- The greatest naked-eye astronomer of the pre-telescope age.
Nova of 1572
- Bright "New Star" (Nova Stella) in Cassiopaeia
- Failed to measure a parallax for the Nova
- Must be in the celestial realm beyond the Moon!
- Saw this as a blow to the Ptolemaic system
- Tycho developed his own "Tychonic" system to replace the
Ptolmaic
Tychonic System
- Hybrid System
- Earth at Center
- Moon and Sun orbit the Earth
- Planets orbit the Sun!
- Full machinery of epicycles, etc., but no equant, like the Copernican system
Uraniborg
- Tycho needed the best astronomical data to prove that his system was correct.
- Built "Uraniborg" (Heavenly Castle) on the island of Hven with royal support.
- Equipped with the best instruments
- Achieved an unprecendented 1-2 arcminute measurement precision
- Became an important center for astronomical research in Europe.
The Lord of Uraniborg
- Astronomical Database
- Positions of 777 stars to 1-2 arcmin precision
- 20 years of precise planetary data
- Great Comet of 1577:
- Showed it was farther away than the Moon and orbiting the Sun!
- Intensive Observations of Mars
- Tried and failed to observe the parallax of Mars
- Amassed data on Mars oppositions
"Let me not seem to have lived in vain"
- Tycho had a falling out with the new Danish king, finally leaving Denmark in 1597.
- 1599
- Appointed Imperial Mathematicus at Prague
- 1600
- Hired Johannes Kepler as his assistant
- 1601
- Died in Prague, Kepler took his place
Johannes Kepler (1571 - 1630)
- Brilliant German Mathematician
- Staunch Copernican
- Convinced the Universe was governed by physical laws
- Obsessed with finding harmony in the heavens
- Had a genius for data analysis
- Inherited Tycho's data and post as Imperial Mathematicus in 1601.
The Motions of Mars
- Mars was the key to unlocking the secrets of planetary motion
- Kepler began analyzing the orbit of Mars in 1601. It took him 4 years
- Started by determining the orbit of the Earth using successive oppositions of Mars
- Fit an off-center circle (i.e. not centered on the Sun) to the first 4 data points.
- A fifth test data point did not fit by eight arcminutes!
The Watershed
- Kepler listened to the data
- Knew Tycho's data were accurate to 1-2 arcminutes
- Kepler questioned his assumptions:
- Forced to abandon uniform circular motion
- Concluded Mars' orbit was not a circle
- Published the results in 1609 (Astronomia Nova)
1st Law of Planetary Motion
- The orbits of the planets are ellipses with the Sun at one focus
- Ellipses are characterized by two numbers:
- Semimajor Axis (a): size of the longest axis
- Eccentricity (e): shape of the ellipse (deviation from a perfect circle)
- Orbit of Mars:
- a = 1.5237 AU, e = 0.0934
2nd Law of Planetary Motion
- The line joining the Sun and the planet sweeps out equal areas in equal times
- Planets move fastest at Perihelion
- Planets move slowest at Aphelion
- Kepler's Second Law provides a geometric description of the change in speed.
- It completely eliminates epicycles
3rd Law of Planetary Motion
- The square of a planet's orbital period is proportional to the cube of the semimajor axis of the orbit.
- Expressed mathematically:
- P2 = a3
- P = Period in years, a = semimajor axis in AU
Empirical Laws
- Kepler's Laws are Empirical Laws
- They describe how the planets move
- They do not explain why they move that way
- Not yet Physical Laws
- Kepler made a start, but he had incorrect ideas about forces
- Kepler's thinking was strongly motivated by his notions of universal harmony.
- Correct explanation had to wait until the work of Isaac Newton
See A Note about Graphics to learn
why some of the graphics shown in the lectures are not reproduced with
these notes.
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Updated: 2007 January 18
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