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

A small block $B$ fits inside a slot cut in arm $…

Question

Answered step-by-step

Problem 60 Easy Difficulty

A semicircular slot of 10 -in. radius is cut in a flat plate which rotates about the vertical $A D$ at a constant rate of $14 \mathrm{rad} / \mathrm{s}$. A small, $0.8-\mathrm{lb}$ block $E$ is designed to slide in the slot as the plate rotates. Knowing that the coefficients of friction are $m_{x}=0.35$ and $m_{k}=0.25,$ determine whether the block will slide in the slot if it is released in the position corresponding to $(a) \mathrm{u}=80^{\circ},(b) \mathrm{u}=40^{\circ} .$ Also determine the magnitude and the direction of the friction force exerted on the block immediately after it is released.


Video Answer

Solved by verified expert

preview
Numerade Logo

This problem has been solved!

Try Numerade free for 7 days

Sheh Lit Chang
University of Washington

Like

Report

Textbook Answer

Official textbook answer

Video by Sheh Lit Chang

Numerade Educator

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

More Answers

02:18

Salamat Ali

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
Elyse Gonzalez

Cornell University

LB
Liev Birman
Farnaz Mohseni

Simon Fraser University

Jared Enns

University of Winnipeg

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

07:14

A small block $B$ fits ins…

06:20

A $0.5-\mathrm{kg}$ block …

03:58

'A solid block having…

01:47

The member $O A$ rotates a…

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

Yes. Question. We have this set up. Hey, there's a block. Small block V Sweeter inside. Uh, this, uh, slot thing. Okay. And then we are told that the speed he is 1.4 m close. Second for data, uh, is in between potato between zero degrees, 250 degrees. Okay. And then we know that the block we are given that lock flights when data, it goes 250 degrees. Okay. And then the rotation is in constant read. Mm. So this means there's no tangential acceleration. Okay, so the question wants us to find a coefficient of static friction between the block and the slot. Okay. Okay. So, uh, using the given information, KB. So we will only look at the situation when data, it goes 250 degrees. Okay. And we look at the free body diagram of the block. Oh, okay. So at 100 GPS, it will look something like this. This is, uh, and large region of the block. And then, uh, so you draw this, um, political lying. Okay, so this is 30 degrees on the block. You have the weight mg. Okay. You have the normal force, but in this direction. Okay, then you have friction pointing in this direction. Yeah. Okay. So, um, as mentioned just now, there's no tangential acceleration. 80 0. I'm going also going to, uh, indicator acceleration. The acceleration. There is a normal component. Yeah, because the whole thing is in secular motion. Okay, but just at the speed is constant. So there's no tangential acceleration that you have, uh, acceleration along the normal components, which is the centripetal acceleration. Okay, so, uh, the e n s. We square overrode A B is 1.4 and then roll is your country. Okay, so this is Oh, something that we need to use later. You calculate needs to be 6.533 You know this post second square, Okay. And then from the free body diagram, Okay. I'm going to use a coordinate system that looks like this accent. Why, then, using you then second law, it forces along the X direction will give us an a N k. So I will write mg. Of course. I 30 degrees okay. Minus f equals two and the square. We're okay. O m a n key. Yeah. So how do I know that it is co sign. So the angle 30 degrees is with the vertical. It is also this angle here. The new single here is 30 degrees. Uh huh. And then, uh, forces along the y is zero. Okay, because 1/10 century zero. Okay, so if you look at the diagram again, then we have ah mg sine 30 degrees. It was too. Uh okay, then, Uh uh, fiction. It's going to be equal to u S n. Okay, so, uh, problem. Oh, from equation one. Okay. And combined to he This is what we are going to have mg co sign 30 degrees minus us. And because two and we square over All right. And then n is mg side 30 degrees so you can cancel the M. Yeah. And then you make, uh, us Julie. Sorry. 30 degrees and the left hand side. And you get G cause I d. Degrees, right? Yes. We square overall. T So your ass with Jesse to cause i d degrees finance lease where we roll with it. Bye bye. Do you say the D degrees? Okay. Very kind. Who in the numbers the company is You get 0.400 So this is that coefficient of static friction. And that's all for this question.

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
75
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
Elyse Gonzalez

Cornell University

LB
Liev Birman

Numerade Educator

Farnaz Mohseni

Simon Fraser University

Jared Enns

University of Winnipeg

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

07:14

A small block $B$ fits inside a slot cut in arm $O A$ that rotates in a vertica…

06:20

A $0.5-\mathrm{kg}$ block $B$ slides without friction inside a slot cut in arm …

03:58

'A solid block having a weight of 160 N is placed at a distance of 1.40 m from …

01:47

The member $O A$ rotates about a horizontal axis through $O$ with a constant co…

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