Download the App!

Get 24/7 study help with the Numerade app for iOS and Android! Enter your email for an invite.

Sent to:
Search glass icon
  • Login
  • Textbooks
  • Ask our Educators
  • Study Tools
    Study Groups Bootcamps Quizzes AI Tutor iOS Student App Android Student App StudyParty
  • For Educators
    Become an educator Educator app for iPad Our educators
  • For Schools

Problem

Show that the radius $r$ of the orbit of a moon o…

Question

Answered step-by-step

Problem 80 Easy Difficulty

Communication satellites are placed in a geosynchronous orbit, i.e. in a circular orbit such that they complete one full revolution about the earth in one sidereal day $(23.934 \mathrm{h})$, and thus appear stationary with respect to the ground. Determine $(a)$ the altitude of these satellites above the surface of the earth, $(b)$ the velocity with which they describe their orbit. Give the answers in both SI and U.S. customary units.


Video Answer

Solved by verified expert

preview
Numerade Logo

This problem has been solved!

Try Numerade free for 7 days

Keshav Singh
Numerade Educator

Like

Report

Textbook Answer

Official textbook answer

Video by Keshav Singh

Numerade Educator

This textbook answer is only visible when subscribed! Please subscribe to view the answer

Related Courses

Physics 101 Mechanics

Vector Mechanics for Engineers: Statics and Dynamics

Chapter 12

Kinetics of Particles: Newton’s Second Law

Related Topics

Newton's Laws of Motion

Discussion

You must be signed in to discuss.
Top Physics 101 Mechanics Educators
Andy Chen

University of Michigan - Ann Arbor

LB
Liev Birman
Marshall Styczinski

University of Washington

Zachary Mitchell

Hope College

Physics 101 Mechanics Courses

Lectures

Video Thumbnail

03:28

Newton's Laws - Intro

Newton's Laws of Motion are three physical laws that, laid the foundation for classical mechanics. They describe the relationship between a body and the forces acting upon it, and its motion in response to those forces. These three laws have been expressed in several ways, over nearly three centuries, and can be summarised as follows: In his 1687 "Philosophiæ Naturalis Principia Mathematica" ("Mathematical Principles of Natural Philosophy"), Isaac Newton set out three laws of motion. The first law defines the force F, the second law defines the mass m, and the third law defines the acceleration a. The first law states that if the net force acting upon a body is zero, its velocity will not change; the second law states that the acceleration of a body is proportional to the net force acting upon it, and the third law states that for every action there is an equal and opposite reaction.

Video Thumbnail

09:37

Newton's Laws Basics - Overview

Isaac Newton (4 January 1643 – 31 March 1727) was an English mathematician, physicist, astronomer, theologian, and author (described in his own day as a "natural philosopher") who is widely recognised as one of the most influential scientists of all time and a key figure in the scientific revolution. His book Philosophiæ Naturalis Principia Mathematica ("Mathematical Principles of Natural Philosophy"), first published in 1687, laid the foundations of classical mechanics. Newton also made seminal contributions to optics, and he shares credit with Gottfried Wilhelm Leibniz for developing the infinitesimal calculus.

Join Course
Recommended Videos

04:53

Communication satellites a…

07:57

Communication satellites a…

02:14

Communication satellites a…

02:29

Geostationary satellites a…

04:57

While describing a circula…

02:46

Communications satellites …

05:32

Geosynchronous orbits Seve…

Watch More Solved Questions in Chapter 12

Problem 1
Problem 2
Problem 3
Problem 4
Problem 5
Problem 6
Problem 7
Problem 8
Problem 9
Problem 10
Problem 11
Problem 12
Problem 13
Problem 14
Problem 15
Problem 16
Problem 17
Problem 18
Problem 19
Problem 20
Problem 21
Problem 22
Problem 23
Problem 24
Problem 25
Problem 26
Problem 27
Problem 28
Problem 29
Problem 30
Problem 31
Problem 32
Problem 33
Problem 34
Problem 35
Problem 36
Problem 37
Problem 38
Problem 39
Problem 40
Problem 41
Problem 42
Problem 43
Problem 44
Problem 45
Problem 46
Problem 47
Problem 48
Problem 49
Problem 50
Problem 51
Problem 52
Problem 53
Problem 54
Problem 55
Problem 56
Problem 57
Problem 58
Problem 59
Problem 60
Problem 61
Problem 62
Problem 63
Problem 64
Problem 65
Problem 66
Problem 67
Problem 68
Problem 69
Problem 70
Problem 71
Problem 72
Problem 73
Problem 74
Problem 75
Problem 76
Problem 77
Problem 78
Problem 79
Problem 80
Problem 81
Problem 82
Problem 83
Problem 84
Problem 85
Problem 86
Problem 87
Problem 88
Problem 89
Problem 90
Problem 91
Problem 92
Problem 93
Problem 94
Problem 95
Problem 96
Problem 97
Problem 98
Problem 99
Problem 100
Problem 101
Problem 102
Problem 103
Problem 104
Problem 105
Problem 106
Problem 107
Problem 108
Problem 109
Problem 110
Problem 111
Problem 112
Problem 113
Problem 114
Problem 115
Problem 116
Problem 117
Problem 118
Problem 119
Problem 120
Problem 121
Problem 122
Problem 123
Problem 124
Problem 125
Problem 126
Problem 127
Problem 128
Problem 129
Problem 130
Problem 131
Problem 132
Problem 133

Video Transcript

for the gravitational force between the earth on the satellite and it's circular orbit about art. We have that the force acting between the earth in the satellite is G capital M the mass of the Earth little M the mass of the satellite over there, separation off the centers R squared. And because of the circular orbit off the satellite, he forced you to the center of the centripetal force. Is MV squared over R. So from here, if you rearrange, we can get the speed of the satellite V to be the square root off G mm over our. But we also know that V Times Tour is equal to two pi r. So tall is the period off one orbit of the satellite and two pi r is the circumference or the total distance that this satellite recover. And if we square both sides, we get that V squared. Torre squared is equal to G and tall squared over our and this is equal to for pi squared r squared And so we can rearrange this equation and fine are so we get our cute We multiply both sides by our is equal to G am toss squared over for pi squared. Until then. From here we can see that the separation between the earth and the satellite is G I am Torre squared over four pi squared to the power off one third. So the cube root off gm tall, squared over four pi squared. Now that we have an expression for the separation, we can substitute our data into this equation. So Tor, the period off the satellite is 23 0.934 hours and this is equal to 86 point 16 24 times 10 to the three in seconds. So firstly, we're going to use S I units in S I units G is equal to nine for 81 m per square. Second, the radius of the earth are is equal to six 0.37 times 10 to the 6 m G times M, we know is equal to the gravitational acceleration little G and the square of the radius of the earth elsewhere. And this is equal to nine when 81 time, six 0.37 times 10 to the six squid. And this becomes 398 0.6 times 10 to the public 12 cubic meter per square second. So therefore, using the equation above, we confined our in S I units to be 398 0.0 six times 10 to the 12 That's needs a cube second squared or GM times 86 point 16 24 times 10 to the three squared over for hi squared and all of this to the power one third. And so if you perform this, we get are to be 42.145 times 10 to the 6 m. So the separation between the satellite and the sent off the earth It's 42.145 times 10 to the 6 m. What? We want to calculate the altitude. The altitude off the satellite above the earth will call it H is equal to this distance minus the radius off the earth since the altitude is the height above ground, not the height above the center off the earth. So this is if we take this value minus big are we get this to be 35 point 775 times 10 to the 6 m. So this is actually 35,000 800 kilometers for the altitude of the satellite is 35,800 kilometers and we can redo the calculation using US customer units where G is 32.2 ft, the square second and the ladies off the earth big our is 3960 miles which is 20,909 times 10 to the 6 ft. And if we do the calculation or we simply convert this answer from kilometers two miles, we get that this is 35,800 kilometers or 22,200 miles in altitude. So for pardon me, we wish to calculate the units and getting us students so V is equal to the square root off GM overall and again, we know these values. So that's the square root off 398 when 06 I can stand to the 12 in S I units over art which is funny to point 145 times 10 to the sixth in meters and so we get the speed of the satellite to be 3.7 times 10 to the three meters per second and this is simply 3.7 kilometers per second. So we can do the calculation again and we get reconvert. These are units into US units and we get the velocity to be 10 0.9 times 10 to the power three feet the second.

Get More Help with this Textbook
Ferdinand Beer, Jr., E. Russell Johnston, David Mazurek

Vector Mechanics for Engineers: Statics and Dynamics

View More Answers From This Book

Find Another Textbook

Study Groups
Study with other students and unlock Numerade solutions for free.
Math (Geometry, Algebra I and II) with Nancy
Arrow icon
Participants icon
74
Hosted by: Ay?Enur Çal???R
Math (Algebra 2 & AP Calculus AB) with Yovanny
Arrow icon
Participants icon
50
Hosted by: Alonso M
See More

Related Topics

Newton's Laws of Motion

Top Physics 101 Mechanics Educators
Andy Chen

University of Michigan - Ann Arbor

LB
Liev Birman

Numerade Educator

Marshall Styczinski

University of Washington

Zachary Mitchell

Hope College

Physics 101 Mechanics Courses

Lectures

Video Thumbnail

03:28

Newton's Laws - Intro

Newton's Laws of Motion are three physical laws that, laid the foundation for classical mechanics. They describe the relationship between a body and the forces acting upon it, and its motion in response to those forces. These three laws have been expressed in several ways, over nearly three centuries, and can be summarised as follows: In his 1687 "Philosophiæ Naturalis Principia Mathematica" ("Mathematical Principles of Natural Philosophy"), Isaac Newton set out three laws of motion. The first law defines the force F, the second law defines the mass m, and the third law defines the acceleration a. The first law states that if the net force acting upon a body is zero, its velocity will not change; the second law states that the acceleration of a body is proportional to the net force acting upon it, and the third law states that for every action there is an equal and opposite reaction.

Video Thumbnail

09:37

Newton's Laws Basics - Overview

Isaac Newton (4 January 1643 – 31 March 1727) was an English mathematician, physicist, astronomer, theologian, and author (described in his own day as a "natural philosopher") who is widely recognised as one of the most influential scientists of all time and a key figure in the scientific revolution. His book Philosophiæ Naturalis Principia Mathematica ("Mathematical Principles of Natural Philosophy"), first published in 1687, laid the foundations of classical mechanics. Newton also made seminal contributions to optics, and he shares credit with Gottfried Wilhelm Leibniz for developing the infinitesimal calculus.

Join Course
Recommended Videos

04:53

Communication satellites are placed in a geosynchronous orbit, i.e., in a circu…

07:57

Communication satellites are placed in a geosynchronous orbit, i.e., in a circu…

02:14

Communication satellites are placed in a geosynchronous orbit - that is, in a c…

02:29

Geostationary satellites are always remaining about the same path on equator, i…

04:57

While describing a circular orbit, 185 mi above the surface of the earth, a spa…

02:46

Communications satellites are placed in circular orbits where they stay directl…

05:32

Geosynchronous orbits Several satellites in Earth's equatorial plane have nearl…

Add To Playlist

Hmmm, doesn't seem like you have any playlists. Please add your first playlist.

Create a New Playlist

`

Share Question

Copy Link

OR

Enter Friends' Emails

Report Question

Get 24/7 study help with our app

 

Available on iOS and Android

About
  • Our Story
  • Careers
  • Our Educators
  • Numerade Blog
Browse
  • Bootcamps
  • Books
  • Notes & Exams NEW
  • Topics
  • Test Prep
  • Ask Directory
  • Online Tutors
  • Tutors Near Me
Support
  • Help
  • Privacy Policy
  • Terms of Service
Get started