13.4 Satellite Orbits and Energy
Circular orbits as centripetal motion under gravity, giving speed and period at a given radius plus the energy needed to change orbit.
University Physics Volume 1, 13.4 Satellite Orbits and Energy
9 exercises
13.4 Exercise 1
By what factor must the radius change to reduce the orbital velocity of a satellite by one-half? By what factor would this change the period?
13.4 Exercise 2
There is another consideration to this last calculation of . We derived the equation assuming that the satellite orbits around the center of the astronomical body at the same radius used in the expression for the gravitational force between them. What assumption is made to justify this? Earth is about 81 times more massive than the Moon. Does the Moon orbit about the exact center of Earth?
13.4 Exercise 3
Galaxies are not single objects. How does the gravitational force of one galaxy exerted on the “closer” stars of the other galaxy compare to those farther away? What effect would this have on the shape of the galaxies themselves?
13.4 Exercise 5
Many satellites are placed in geosynchronous orbits. What is special about these orbits? For a global communication network, how many of these satellites would be needed?
13.4 Exercise 7
Two planets in circular orbits around a star have speeds of v and 2v. (a) What is the ratio of the orbital radii of the planets? (b) What is the ratio of their periods?
13.4 Exercise 9
(a) What is the orbital radius of an Earth satellite having a period of 1.00 h? (b) What is unreasonable about this result?
13.4 Exercise 11
Find the mass of Jupiter based on the fact that Io, its innermost moon, has an average orbital radius of 421,700 km and a period of 1.77 days.
13.4 Exercise 13
(a) In order to keep a small satellite from drifting into a nearby asteroid, it is placed in orbit with a period of 3.02 hours and radius of 2.0 km. What is the mass of the asteroid? (b) Does this mass seem reasonable for the size of the orbit?
13.4 Exercise 15
The Sun orbits the Milky Way galaxy once each , with a roughly circular orbit averaging a radius of light-years. (A light-year is the distance traveled by light in 1 year.) Calculate the centripetal acceleration of the Sun in its galactic orbit. Does your result support the contention that a nearly inertial frame of reference can be located at the Sun? (b) Calculate the average speed of the Sun…
Adapted from University Physics Volume 1 © 2016 Rice University. Licensed under CC BY 4.0. Source: University Physics Volume 1. Imported at revision db44eb9.