Chapter 4: Problem 15
What are Kepler's three laws? Why are they important?
Chapter 4: Problem 15
What are Kepler's three laws? Why are they important?
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Get started for freeSuppose that you traveled to a planet with 4 times the mass and 4 times the diameter of the Earth. Would you weigh more or less on that planet than on Earth? By what factor?
At what point in a planet's elliptical orbit does it move fastest? At what point does it move slowest? At what point does it sweep out an area at the fastest rate?
A comet orbits the Sun with a sidereal period of \(64.0\) years. (a) Find the semimajor axis of the orbit. (b) At aphelion, the comet is \(31.5\) AU from the Sun. How far is it from the Sun at perihelion?
How did the models of Aristarchus and Copernicus explain the retrograde motion of the planets?
Imagine a planet like the Earth orbiting a star with 4 times the mass of the Sun. If the semimajor axis of the planet's orbit is \(1 \mathrm{AU}\), what would be the planet's sidereal period? (Hint: Use Newton's form of Kepler's third law. Compared with the case of the Earth orbiting the Sun, by what factor has the quantity \(m_{1}+m_{2}\) changed? Has \(a\) changed? By what factor must \(P^{2}\) change?)
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