Physlet Illustration: Kepler's Second Law |
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A planet orbits a star under the influence of gravity. The distance grid is in Astronomical Units
(AU), and the time is shown in years. The animation begins from the point
of aphelion, and the total area swept out by the planet's orbit is given in AU2. Can you verify Kepler's Second Law?
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Hints:
- Starting at t = 0, run the animation for a certain time
interval. How much area has been swept out by the planet in this time interval?
- Now, continue the animation for a second time interval of equal
duration. How much total area has now been swept out? How much area,
then, was swept out in the second time interval?
- Can you verify Kepler's First Law, as well? What is the eccentricity
of the elliptical orbit?
- Turn on the Interactive Help. How does the planet's speed (shown in
AU/yr) vary as it
executes its orbit?
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Reference
See Walker, Section 12-3
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Illustration written by Steve Mellema
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