The Solar System
The Solar System
9th Edition
ISBN: 9781305804562
Author: Seeds
Publisher: Cengage
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Chapter 4, Problem 11RQ
To determine

Whether epicycle or deferent travels in uniform circular motion as viewed from particular point. Whether the uniform circular motions have same speed and in same directions.

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Describe three propositions, now known as Kepler’s laws of planetary motion?
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.
Kepler's Third Law and Newton's Law of Universal Gravitation (a) Use Newton's Universal Law of Gravitation and what you know about centripetal acceleration/force to derive Kepler's Third Law for a planet in a circular orbit about the sun: T² = Kr³ K = constant = 4²/GM where T is the orbital period of the planet (the time for one complete orbit), r is the radius of the planet's orbit, M is the mass of the sun, and G is the universal gravitational constant. (b) Determine the metric system units of K and show that they make the units of T² – Kr³ work out correctly. (c) The earth orbits the sun once per year (365 days) and its average orbital radius is 1.50 x 10¹¹ m. Use this information and Kepler's Third Law to estimate the mass of the sun in kilograms. [answer: about 2 x 10³⁰ kg] (d) The radius of the sun is about 7 x 108 m. Use this radius and the mass of the sun estimated in part (c) to estimate the acceleration of an object near the surface of the sun. [answer: about 300 m/s²] F₂ =G…

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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