Universe
Universe
11th Edition
ISBN: 9781319039448
Author: Robert Geller, Roger Freedman, William J. Kaufmann
Publisher: W. H. Freeman
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Chapter 4, Problem 6Q
To determine

The explanation provided by Aristarchus and Copernicus for the retrograde motion of the planets.

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A planet revolves around a certain star. At one point in the planet's orbit, called periapsis, it passes much closer to the star. Which of the following statements about periapsis is true?   The planet's orbital period becomes shorter after every periapsis.   The planet's orbital period becomes longer after every periapsis.   The planet orbits with a slower speed during periapsis.   The planet orbits with a greater speed during periapsis.
Kepler's 1st law says that our Solar System's planets orbit in ellipses around the Sun where the closest distance to the Sun is called perihelion. Suppose I tell you that there is a planet with a perihelion distance of 2 AU and a semi-major axis of 1.5 AU. Does this make physical sense? Explain why or why not.
Which of the following statements is supported by Kepler's laws of planetary motion?   Earth orbits the Sun at a constant speed, never speeding up or slowing down.   Earth's orbit is a perfect circle, with the Sun located at the center of the circle.   Earth orbits the Sun at a slightly faster speed every year.   Earth has an elliptical orbit, with the Sun located at one focus of the ellipse.
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Kepler's Three Laws Explained; Author: PhysicsHigh;https://www.youtube.com/watch?v=kyR6EO_RMKE;License: Standard YouTube License, CC-BY