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Extrasolar planets and Kepler’s Third Law

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Presentation on theme: "Extrasolar planets and Kepler’s Third Law"— Presentation transcript:

1 Extrasolar planets and Kepler’s Third Law
AF. May 2015

2 Nose lost in 1566 following a sword duel with third cousin Manderup Parsberg over the legitimacy of a mathematical formula! Nicolaus Copernicus Tycho Brahe Johannes Kepler Isaac Newton

3 Johannes Kepler 1571-1630 Polar equation of ellipse This is a constant
Equal areas swept out in equal times Eccentricity of ellipse Orbital period P Johannes Kepler

4 Radii of planets not to scale!
Neptune Kepler’s Third Law Johannes Kepler Orbital period P /years Uranus Mercury, Venus, Earth, Mars Saturn Jupiter Semi-major axis of orbit a / AU

5 Planet and Solar masses
Isaac Newton ( ) developed a mathematical model of Gravity which predicted the elliptical orbits proposed by Kepler Planet and Solar masses Force of gravity Semi-major axis Polar equation of ellipse Semi-minor axis Eccentricity of ellipse Orbital period P

6 Kepler’s Third Law semi-major axis of elliptical orbit

7

8 Vertical intercept is very
close to ln(365) = 5.90 Gradient is 1.49, not far off the Kepler #3 prediction of 3/2

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12 Earth-like candidates?


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