Phys1101 - Introductory Physics 1
Phys1101 - Introductory Physics 1
College of Liberal Arts & Sciences

  • Introduction
  • Lecture 01
  • Lecture 02
    • Lecture 2, Part 1: Announcements
    • Lecture 2, Part 2: Units
    • Lecture 2, Part 3: Vector Introduction
    • Lecture 2, Part 4: Adding Vectors Graphically
    • Lecture 2, Part 5: Vector Addition Examples
    • Lecture 2, Part 6: Vector Component Introduction
    • Lecture 2, Part 7: Trigonometry
  • Lecture 03
    • Lecture 3, Part 1: Introduction
    • Lecture 3, Part 2: Where Were We
    • Lecture 3, Part 3: Vector Components in Detail
    • Lecture 3, Part 4: Scalar Component Description
    • Lecture 3, Part 5: Example of Finding Scalar Components
    • Lecture 3, Part 6: Scalar Component Addition
    • Lecture 3, Part 7: Scalar Addition Example
    • Lecture 3, Part 8: Motion Diagrams
  • Lecture 04
    • Lecture 4, Part 1: Introduction
    • Lecture 4, Part 2: Where Were We
    • Lecture 4, Part 3: Location Location Location …
    • Lecture 4, Part 4: How Fast ??? What Direction ???
    • Lecture 4, Part 5: Speeding Up? Slowing Down?
    • Lecture 4, Part 6: What Happens at a Turning Point?
  • Lecture 05
    • Lecture 5, Part 01: Introduction
    • Lecture 5, Part 02: Where Were We
    • Lecture 5, Part 03: Big Picture:  1D Kinematics
    • Lecture 5, Part 04: Kinematic Problem Solving Steps
    • Lecture 5, Part 05: Example 1
    • Lecture 5, Part 06: Example 2
    • Lecture 5, Part 07: Example 3
    • Lecture 5, Part 08: Free Fall
    • Lecture 5, Part 09: Free Fall and Kinematic Equations
    • Lecture 5, Part 10: Example 4
    • Lecture 5, Part 11: Example 5
  • Lecture 06
    • Lecture 6, Part 1: Introduction
    • Lecture 6, Part 2: Where Were We
    • Lecture 6, Part 3: Reading Quiz
    • Lecture 6, Part 4: Graph Basics
    • Lecture 6, Part 5: Practice Makes Perfect…
    • Lecture 6, Part 6: The Tangent Line
  • Lecture 07
    • Lecture 7, Part 1: Introduction
    • Lecture 7, Part 2: Where Were We
    • Lecture 7, Part 3: 2D Motion Diagrams
    • Lecture 7, Part 4: Trajectories
    • Lecture 7, Part 5: Why Work With Components…
    • Lecture 7, Part 6: Key Vectors in 2D
    • Lecture 7, Part 7: Watching 2D Motion
    • Lecture 7, Part 8: Dropping Versus Firing…
  • Lecture 08
    • Lecture 8, Part 1: Introduction
    • Lecture 8, Part 2: Where Were We
    • Lecture 8, Part 3: 2D Kinematic Problems:  The Big Picture
    • Lecture 8, Part 4: 2D Kinematic Problem Solving Steps
    • Lecture 8, Part 5: Example – Part a
    • Lecture 8, Part 6: Example – Part b
    • Lecture 8, Part 7: Your Turn
  • Lecture 09
    • Lecture 9, Part 1: Introduction
    • Lecture 9, Part 2: Where Were We
    • Lecture 9, Part 3: What is Special About Projectile Motion?
    • Lecture 9, Part 4: Example Part a
    • Lecture 9, Part 5: Example Part b
    • Lecture 9, Part 6: Example Part c
    • Lecture 9, Part 7: Your Turn
  • Lecture 10
    • Lecture 10, Part 1: Introduction
    • Lecture 10, Part 2: Where Were We
    • Lecture 10, Part 3: Dynamics:  Why Does Velocity Change?
    • Lecture 10, Part 4: Physical Interpretation of Newton’s Laws
    • Lecture 10, Part 5: What is a Force?
    • Lecture 10, Part 6: Mathematics of Newton’s 2nd Law
  • Lecture 11
    • Lecture 11, Part 1: Introduction
    • Lecture 11, Part 2: Where Were We
    • Lecture 11, Part 3: Free Body Diagram and Vector Nature of Newton’s 2nd Law
    • Lecture 11, Part 4: Common Forces:  Weight
    • Lecture 11, Part 5: Common Forces:  Tension
    • Lecture 11, Part 6: Common Forces:  Normal Force
    • Lecture 11, Part 7: Common Forces:  Friction
    • Lecture 11, Part 8: Problem Solving Steps
    • Lecture 11, Part 9: Example
  • Lecture 12
    • Lecture 12, Part 1: Introduction
    • Lecture 12, Part 2: Where Were We
    • Lecture 12, Part 3: Example 1
    • Lecture 12, Part 4: Example 2
    • Lecture 12, Part 5: Example 3
  • Lecture 13
    • Lecture 13, Part 1: Introduction and Where Were We?
    • Lecture 13, Part 2: Why/When Do We Need Newton’s Third Law?
    • Lecture 13, Part 3: Newton’s 3rd Law
    • Lecture 13, Part 4: Changes To Our Problem-Solving Steps
    • Lecture 13, Part 5: Example 1
    • Lecture 13, Part 6: Ropes and Pulleys
    • Lecture 13, Part 7: Example 2
    • Lecture 13, Part 8: Your Turn
  • Lecture 14
    • Lecture 14, Part 01: Introduction
    • Lecture 14, Part 02: Where Were We ?
    • Lecture 14, Part 03: Uniform Circular Motion:  What You Need To Know
    • Lecture 14, Part 04: Example 1
    • Lecture 14, Part 05: Example 2
    • Lecture 14, Part 06: Example 3
    • Lecture 14, Part 07: Optional Roller Coaster Example
    • Lecture 14, Part 08: Satellite Example
    • Lecture 14, Part 09: The Universal Law of Gravitation
    • Lecture 14, Part 10: Satellite Example Continued
  • Lecture 15
    • Lecture 15, Part 1: Introduction and Where Were We?
    • Lecture 15, Part 2: Energy Conservation:  The Basics
    • Lecture 15, Part 3: How Do You Calculate the Net Work?
    • Lecture 15, Part 4: New Problem Solving Steps
    • Lecture 15, Part 5: Example 1
    • Lecture 15, Part 6: Example 2
    • Lecture 15, Part 7: Last Example
    • Lecture 15, Part 8: Final Quiz Questions…
  • Lecture 16
    • Lecture 16, Part 1: Introduction and Where Were We?
    • Lecture 16, Part 2: Defining Our New “Energy Conservation Starting Equation”
    • Lecture 16, Part 3: Defining Mechanical Energy
    • Lecture 16, Part 4: New Problem Solving Steps
    • Lecture 16, Part 5: First Example
    • Lecture 16, Part 6: Second Example
    • Lecture 16, Part 7: Last Example
    • Lecture 16, Part 8: Redo Example From Last Lecture
  • Lecture 17
    • Lecture 17, Part 1: Lecture
  • Lecture 18
    • Lecture 18, Part 1: Introduction and Where Were We?
    • Lecture 18, Part 2: Momentum Change of a Single Object
    • Lecture 18, Part 3: Conservation of Momentum
  • Lecture 19
    • Lecture 19, Part 1: Introduction and Where Were We?
    • Lecture 19, Part 2: Let’s Start With Another Example
    • Lecture 19, Part 3: Elastic Collisions
    • Lecture 19, Part 4: Remaining Quiz Questions
  • Lecture 20
    • Lecture 20, Part 1: Introduction and Where Were We?
    • Lecture 20, Part 2: Rotational Kinematics:  The Basics
    • Lecture 20, Part 3: Examples
  • Lecture 21
    • Lecture 21, Part 1: Introduction and Where Were We?
    • Lecture 21, Part 2: Describing Motion ALONG the Circular Path…
    • Lecture 21, Part 3: Examples
    • Lecture 21, Part 4: Rolling Motion
  • Lecture 22
    • Lecture 22, Part 1: Introduction and Where Were We?
    • Lecture 22, Part 2: A Net Torque Causes Angular Acceleration
    • Lecture 22, Part 3: Torque Example
    • Lecture 22, Part 4: Equilibrium Example
    • Lecture 22, Part 5: Moment of Inertia
    • Lecture 22, Part 6: Non-Equilibrium Example
    • Lecture 22, Part 7: Another Example
  • Lecture 23
    • Lecture 23, Part 1: Introduction and Where Were We?
    • Lecture 23, Part 2: The Basics of Oscillatory Motion
    • Lecture 23, Part 3: Hooke’s Law
    • Lecture 23, Part 4: Kinematics of Simple Harmonic Motion
    • Lecture 23, Part 5: Example
  • Lecture 24
    • Lecture 24, Part 1: Lecture
  • Lecture 25
    • Lecture 25, Part 1: Introduction
    • Lecture 25, Part 2: The Basics of Wave Motion
    • Lecture 25, Part 3: Motion of a Particle on a Wave
    • Lecture 25, Part 4:  Motion of The Wave Crest
    • Lecture 25, Part 5: Examples
Lecture 21 » Lecture 21, Part 4: Rolling Motion

Lecture 21, Part 4: Rolling Motion

https://youtu.be/3b7ncc1O1cA

PHYS 1101: Lecture Twenty-One, Part Four

The last topic for this lecture is the idea of rolling motion. It really ties together these distance quantities that are happening, which are the distance and the motion along the circle when something is rotating and this rotational motion. It really connects it together. This is an example of a wheel rolling across the ground. That’s what we mean by rolling motion. Let me show you an animation to see a very important connection between rolling motion and the motion of this wheel as a whole that you observe. Here’s my wheel in this animation, and it’s going to roll to the right. It’s not slipping as it rolls.

So notice that it starts out with this line pointing right here at the edge of this pause button. I want to let this roll through one revolution and as it rolls forward in one revolution we need to think about the connection between the distance that it travels and this circular motion that has happened. Let’s watch it and I will show you what I mean. I’m going to let it go around one time. Oops. There! Perfect. I stopped it perfectly. Let me grab a snapshot of that and let’s do a little analysis of it.

Okay, there’s the picture. And now I’ve added a line here to remind us of where it started. So, at the start of the problem when that wheel was here, that black line, a scratch on the wheel, if you want to think of it, was pointed straight down. As it rolled to the right, if it didn’t slip, I wanted to point out that as it rolled this surface of the wheel came into contract with the ground as this rolled forward and we let it roll forward one complete cycle. By the time it ended that black line was back to pointing straight down.

If you think carefully about it, in the process of rolling one through one revolution, if this surface of the wheel always stayed in contact with the ground as it rolled forward, then the distance around this wheel has to be the distance along this line. This has to be 2πr, the circumference of the wheel.

If you don’t believe it, imagine you have a sticky line of tape all the way around this wheel. As you roll it out, the tape sticks to the ground. When you roll this one revolution and it moves to the right, you will stick to the ground one layer of this tape that was wrapped around this wheel, it really is true.

Well, let’s think about the rotational characteristics of this wheel. I know, for example, that the tangential velocity of this wheel is equal to the circumference divided by the period. This we learned back in chapter five. I also just argued to you that in the time it takes for this wheel to complete one cycle, it has moved forward this distance of 2πr, and in how long? How long did it take to go around once? Well, it’s the same value of the period. So I am going to write here, to the side, the distance to the right analysis shows that the center of this wheel, if I just followed the general motion of this wheel, that it moved forward the distance of 2πr.

Also, in that same time, the period, the time it takes for the wheel to go through one cycle, we’ll notice that these things are the same. The tangential speed at the edge of the wheel has to be equal to the speed of the center of the wheel, just as you watch that wheel move to the right and translate along. Very important connection that at first isn’t obvious. So let me highlight then this has to equal that because the right sides are equal.

That’s said, or summarized, here in this red box. Let me emphasis, then, that this Vcenter, what I mean by that is, for example that this is the speed of the bike, the speed of the car, it’s the speed of the wheel, the center of the wheel as it moves to the right, that distance over time is equivalent to the tangential speed of the edge of the wheel, that distance over time.

Okay, we can use that important connection in a lot of problems that have to do with rolling motion to connect some of these variables. Let’s do a final example for this lecture. I’ve got a motorcycle that accelerates uniformly from rest and reaches a linear speed of 22 meters per second in a time of 9 seconds. That to me is giving me the information that vcenter is equal to 22 meters per second. I right away can draw the conclusion that that’s vT; that’s the tangential velocity at the edge of my wheel. That’s what the rolling motion analysis immediately tells me.

The radius of the tire is .28. What’s the magnitude of the angular acceleration of each wheel? Here’s my wheel. It’s accelerating.

I’m going to sketch my acceleration in this direction. Just because that will be my nice, positive convention. So I start out with an initial tangential velocity of some value. Let me do here my time, position, and initial tangential velocity. At some later point I have a time, position, and tangential velocity and I have an aT tangential acceleration in between.

What are the knowns that I have? Summarized above, I know that vT is equal to 22 meters per second. I know that my final time is nine seconds. I know the radius of the wheel is .28. What do I want? I need the angular acceleration. Notice that’s not the tangential acceleration, but the angular. So I want Alpha. But I have all this information that’s about the kinematics along the circular path.

From this combination, I can determine what the tangential acceleration is, and then do I know the relationship that connects aT to Alpha? Yeah, I do. I know that aT is equal to r times Alpha. So if I go after aT first, which I am inclined to do because of this kinematic information I have about this kinematics along the circle. Then I can use this equation to get the thing I want: Alpha.

I forgot one more kinematic variable that I need. It’s always helpful; I should be more disciplined about going through my list here to be sure I’m not leaving anything out. The motorcycle does accelerate uniformly from rest up to this speed. If it starts at rest then I know my initial tangential velocity is zero. All of these are zero at this initial instant. And then my final time is 9 seconds. I don’t know about the final path along the wheel. The final tangential speed I do know. It’s 22.

Okay, so let’s take that approach. Can we get aT from the things that we know? And you know what? That equation one is looking really good again. vT is equal to vT0 plus aT times the time. Again, I know a lot of these variables so I can go after aT. This one is zero. aT is going to be just vT divided by time. The final velocity dived by time. That’s 22 meters per second divided by 9 seconds, is 2.44 meters per second squared.

aT now, this relationship can be used to get Alpha. Little algebra rearranging here. Alpha is equal to aT over r. So Alpha is 2.44 meters per seconds2 divided by 0.28 meters. That’s 8.73 radians per second2.

Comment on the units here. The meters cancel. So my equation looks like I’ve got no units in the numerator, divided by seconds2. And that’s what it should like for Alpha in is units. I know then to put back my placeholder of radians per second2. That I have radians. If I had been left with some other unit here another meter or kilogram, something would have been wrong. No units per seconds2, that’s what I am after. That’s a good sign. So there would be the answer to that problem.

So perhaps the important connection to make in this problem was to recognize that it involves rolling motion and connecting the linear speed that’s the motion along the line for this motorcycle as it moves, say, horizontally to the right. Its speedometer reads 22 meters per second, and to recognize that that means that the wheels are going around with a tangential speed that’s also 22 meters per second. That was a critical connection to make in order for us to realize we had a lot of information about this rotational motion of the wheel to figure out this angular acceleration of the wheel or the tire.

Okay, so that’s how the rolling motion information can help you out. That brings us to the end of lecture 21.

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