21st Century Astronomy
21st Century Astronomy
6th Edition
ISBN: 9780393428063
Author: Kay
Publisher: NORTON
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Chapter 4, Problem 16QP
To determine

The fundamental difference between Kepler’s laws and Newton’s laws.

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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.
What is Kepler's first law of planetary motion? The period of a planet's orbit is proportional to its distance from the sun. Planets have circular orbits. Planets have elliptical orbits. The eccentricity of a planet's orbit is proportional to its distance from the sun.
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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Time Dilation - Einstein's Theory Of Relativity Explained!; Author: Science ABC;https://www.youtube.com/watch?v=yuD34tEpRFw;License: Standard YouTube License, CC-BY