Kepler’s Laws of Planetary Motion Bormann Honors Science - 8.
Kepler’s Laws of Planetary Motion
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Transcript of Kepler’s Laws of Planetary Motion
Kepler’s Laws of Planetary Kepler’s Laws of Planetary MotionMotion
Mr. FinnNovember, 2008
BackgroundBackground
• Greek astronomy• Ptolemy• Copernicus• Tycho Brahe• Johannes Kepler
Mars
Greek AstronomyGreek Astronomy
• Planets– “little wanderers” hard to explain
• Mars– red planet = “fiery one”– retrograde motion hardest to explain
• Aristarchus– heliocentric system– explains retrograde motion
Retrograde Motion of MarsRetrograde Motion of Mars
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Ptolemaic SystemPtolemaic System
• The Algamest– geocentric system– orbits = system of epicycles– explains retrograde motion– infinitely malleable
• adjusts to new data• extremely accurate predictions
Copernican SystemCopernican System
• Heliocentric system– planet orbits = circles– not centered on Sun, but points nearby– explains retrograde motion– simple but inaccurate
• not fully consistent with existing data• retains some epicycles
Tycho BraheTycho Brahe
• Observational astronomer– best observatory in Europe at Hven (1576-1596)
– naked-eye observation• telescope by Galileo in 1609
– 20 years of data on planets• Compromise system
– Earth at center– other planets orbit sun
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Johannes KeplerJohannes Kepler
• Mathematician– worked for Brahe 1600-1601
• inherited Brahe’s astronomical data
• Copernican system– Kepler strong believer
• Trials & Tribulations– repeatedly fled wars, religious persecution– mother on trial for witchcraft
Experimental DataExperimental DataKepler’s “War on Mars”Kepler’s “War on Mars”
• Brahe data on Mars– position relative to distant stars for 20yrs from Earth
• Data relative to moving Earth– find positions 1 Martian year apart– Mars at same point in orbit around Sun– seen from different perspectives on Earth
• Earth in different position in its orbit– where lines intersect = position of Mars
• Find orbit without any preconceptions– traces out ellipse!
Theory - Kepler’s LawsTheory - Kepler’s Laws
1. Orbits of planets are ellipses with sun at one foci
2. Planets sweep out equal areas in equal times
3. Relationship between size of orbit & its period
– P a3/2
– P2/a3 = constant
Harmonies in the Heavens
Kepler’s 1st LawKepler’s 1st Law
Sun at one foci
2a
a = semi-major axisperihelion
aphelion
Kepler’s 2nd LawKepler’s 2nd Law
Equal Areas:
A
Equal Times: 1 23 4
planets move faster when closer to the sun
Planet
Sun
Kepler's Third Law
0
50
100
150
200
250
300
0 5 10 15 20 25 30 35 40 45
Semi-Major Axis (AU)
Period (yr)
Kepler’s 3rd LawKepler’s 3rd Law
P a3/2
Unknown to Kepler
Newtonian SynthesisNewtonian Synthesis
• Newton’s Universal Law of Gravity
• Newton’s Laws of Motion– same laws explain heavenly and earthly motion– Aristotle believed two separate laws
€
r F g = −G mM
d2ˆ r d
Grand Synthesis #1Grand Synthesis #1
Celestial MechanicsCelestial Mechanics
• Pierre-Simon Laplace– Treatise on Celestial Mechanics (1799)
• Napoleon - Why is God missing?Why is God missing? – Laplace: “I have no need of that hypothesis.”
• “Je n’ai pas besoin de cette hypothèse.”
• Rise of the “Mechanical UniverseMechanical Universe”
PredictionsPredictions
• Edmund Halley predicts return of comet• Discovery of new planets
– Neptune, Pluto• Effect of planets on each other
– precession of orbits– Mercury partially unexplained