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 22 » Lecture 22, Part 3: Torque Example

Lecture 22, Part 3: Torque Example

https://youtu.be/blm6UUUGNO8

PHYS 1101: Lecture Twenty-Two, Part Three

Let’s walk through this example to see how this might work. My problem here is I’m installing a spark plug in the car, and the manual specifies that it has to be tightened to a torque with a magnitude of 45 Newton meters. So, I need to use the information in this drawing to determine the magnitude of the force that you have to exert on the wrench.

Okay. Let me emphasize a few things. My rotation axis. You got to hone in on that as the first step. That’s going to be the center of my bolt. The r that I need to think about is the length of the line that goes from my center of my rotation axis or my rotation axis out to where the force is applied. That is the length r. Now, to this line r that I need to sketch the perpendicular direction. Perpendicular to that r, I need to find the component of f in this direction. Think of shining a light toward this axis. What’s the shadow that this total force… What’s the shadow that it casts on this axis? That means I need to dash a line straight down toward this axis. This is the part of the force that I need. This is the tangential component. Okay.

So this is finding components again. This is hypotenuse, and this is a component. You’d have to use trigonometry on this force, on this vector, to find this component. The first quiz question here is: what variable would you have to focus on or solve for? What’s it asking? It wants us to determine the magnitude f of the force that you must exert on the wrench. It’s asking for the hypotenuse, but the equation that we’re going to use to determine how large the hypotenuse has to be is the equation that involves just the component, f tangential, the component. So this, I’m going to use my torque equation. For this, I have to substitute in the component of the total force in the tangent direction.

Okay. Question four asks: At the end of the day, what is the variable you need a value for? Okay. Question five: Look carefully at this drawing. You’re told that this is 50 degrees. So, let me just do some similar triangles here and point out for you that then this is 50 degrees. What’s the correct trigonometric equation that represents this component and the hypotenuse and our angle of 50 degrees? So, here I’ve blown up that geometry for you and sketched in r again, from the rotation axis out to where the force is applied. Here’s my hypotenuse. This is the magnitude, my resultant force. I dash in my directions here, one perpendicular to r, and then this one that kind of continues in the direction of r.

What we need is f tangential, which is this component, this side of the right triangle. So, my total f is the hypotenuse. I need a right triangle where this tangent direction is one of my sides of this right triangle. So, let me go in with a really thick blue pen here and write. This force, this component is what you’re after. fT. That’s what has to go into my torque equation. The torque is the radius times fT. What’s the right trigonometric relationship for fT, given this geometry? f is the hypotenuse. That’s the variable you need to solve for.

Okay. So, it’s this torque that causes something to change its rotation, to start spinning faster or slowing down. If you want to see the derivation, I invite you to look through the text. What it’ll show you is that it’s just a rearrangement of our fundamental Newton’s Second Law. Tangential forces cause tangential acceleration. It’s just a connection of these variables to their rotational analogs that leads us to our fundamental equation that we need to highlight here.

Okay. The sum of the torques here has to be all torques, all forces with their location information. The torque implications of all of them have to be considered. Be careful with the sign. You have to represent positive and negative torques here to properly capture competing torques. The denominator is going to be the moment of inertia. I’ll talk to you more about that in just a minute.

The left side of the equation. It’s either going to be zero or some number of real radians per second2. I just took a minute here to rewrite this top statement, because I realized I was a little bit misleading. We want to be really clear. A net torque causes the rotation of an object to change. A net torque causes an angular acceleration, not a velocity, but angular acceleration. This means Alpha… Either the net torque is zero, in which case Alpha is zero. The thing’s in equilibrium.

Or, I can have a net torque, in which case it’s not in equilibrium, and the thing is actually spinning faster or starting to slow down. Remember, if something’s in equilibrium, it could either be sitting there stationary, or don’t forget, it could be sitting there rotating around at a nice constant rate. That also corresponds to Alphas equal to zero, of the thing being in equilibrium. Remember, that was a real subtle point that was difficult to appreciate about Newton’s Second Law. The analog was something could be moving along with a constant velocity and have no net force.

Here are my problem-solving suggestions or hints, kind of sequence of events to try and follow, that will help you get off to a good start when you’re solving these problems. As always, you have to be sure you’ve identified the right object to focus on. In this context, it’s the object that is rotating or might rotate. Isolate that object, and then you’re thinking about torques applied to that object.

What’s the moment of inertia, the variable I, for that object? Which we’ll discuss in a minute here. What’s the angular acceleration for that object? All of these rotation variables are defined by having a very specific axis in the problem. In these problems, you’ll see that it’s either clear what the rotation axis is, it’s given to you, or for equilibrium problems, you’ll see it’s up to you to pick the rotation axis. You’ll see more about that in a minute.

The third step, I would say to slow down and be sure that you’ve in your mind decided if this object is in equilibrium or not, that’ll help you appreciate this distinction. Are you looking for a case if it’s in equilibrium where the torques have to balance? Or is there a real value for the angular acceleration because there is a net torque divided by I? So, our basic equation, maybe I could highlight here for you, turns into really two choices. If it’s in equilibrium, the equation just reduces to the torques adding up to zero. If it’s not in equilibrium, then I have to use this full equation, which I just highlighted again for you.

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