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 13 » Lecture 13, Part 5: Example 1

Lecture 13, Part 5: Example 1

https://youtu.be/2PrWL6VHDmw

PHYS 1101: Lecture Thirteen, Part Five

So here’s our first example. At an airport, luggage is unloaded from the plane into the three cars of the luggage carrier. The acceleration of the carrier is .12 meters per second squared, and we can ignore friction. The coupling bars are very light, says here they have negligible mass. Each cart with luggage has a mass of 39 kilograms. What’s the tension in the coupling bar B?

Okay, do I have to consider this is multiple objects to solve the problem? Well, coupling bar B is the bar here that’s connecting Car 2 to Car 1. All of these objects are accelerating the same in the positive x direction; let’s call it to the right. So, the objects are all moving the same, they’re not, there isn’t any motion between them, but it satisfies that second bullet that I pointed out.

I’m being asked about a force between these objects, namely the coupling bar. Whatever pull the coupling bar is putting on Car 1, it’s going to have the same magnitude of pull on Car 2. I can think of this coupling bar as a rope, in the tensions in that bar and that tension is going to mean the same pull on Car 1 as on Car 2. So I do have to consider them as multiple objects.

I’m going to have to think about Newton’s Third Law as I work the problem. Sometimes it helps to decide what objects to focus on by very early on in the problem, deciding what it is you need a value for.

So, beside here I’m going to write a note right away that I’m after what I’m going to call Tension 2. I’m after the tension in coupling bar 2, that’s the pull to the right on Car 2, it’s another way, it’s the pull to the left on Car 1. This is the variable I’m going to use to represent the tension in that coupling bar. Okay, given that’s the focus, this is a force between these two objects.

I’m going to start working with Newton’s Second Law for one of these objects. Which one to pick? Well, perhaps your eyes are first drawn to Car 1. Let’s flesh it out, let’s walk through Newton’s Second Law applied to Car 1 and see if that gets us what we need, the tension in the coupling car. It’s very common in these Third Law problems, or these more involved problems, that your first approach might not be the most efficient, or the way to go. You’ll see what I mean by that in a minute.

We’re going to start out focusing on Car 1, but I’m going to have you soon realize and appreciate that, you know what, we need to backtrack. Focusing on Car 2, which also experiences this force, is going to be a better way to go for us.

But let’s start out assuming we, naively, our eye was drawn to Car 1. We knew we needed to start and focus on one of these two objects, because these are the, those that are experiencing the force that we’re after. So for Car 1, my acceleration is to the right, that’s going to be my positive x direction. And it has a value of, I’ll jot that down over here, 0.12 meters per second squared. So that’s the consideration for the left side of my equation.

Let’s draw the free body diagram from Car 1 to think about the f net, the net forces. So, here’s my car, drawn as this red object that I’m focused on. What are the forces? I’ve got the weight of the car, I have the normal force. And going around the object, I’ve already got the push of the ground up on the right side for Car 1. I have the coupling bar that’s attached to the jeep. I’m going to call that Tension 1; I’ll jot that in my picture above here. As I continue around, nothing touching the top, when I get to the back end of the car, I have Tension 2, due to this rope or the coupling bar at the end.

I intentionally drew this force to be a little bit larger than that, so I have an fnet consistent with my picture. So, as always, when I apply Newton’s Second Law, it’s really these equations that I mathematically think about. The vertical and the horizontal acceleration m forces and are they consistent with Newton’s Second Law?

These, this motion in these objects are not accelerating up down, only horizontally, so my y equation, which just tells me what I already know, namely that my forces up down have to balance. So that’s my visual check in equating the normal force and the gravity force.

All the action’s happening horizontally, so it’s the a(x) equation that I would look to. Well whatever is causing this .12 meters per second squared acceleration, that’s a result of the balance of the positive tension to the right, minus the tension force that’s to the left, divided by m. This is the value I’m after, and I know the number for the acceleration, I know the mass of each car, but I don’t know the tension in this coupling bar that’s due to the jeep pulling on it.

Now when you run into a situation like that, my instincts then tell me, well, because this is a force between this object and the jeep, let’s now do, apply Newton’s Second Law to the jeep. Well, the jeep is going to have to have some larger force to the right that overcomes the same T1 that’s pulling on the jeep to the left.

That force, technically comes from the interaction of the tires with the ground, and it’s the friction force of the ground that accounts for that. But I don’t know anything about those details to solve that, so I kind of run into a dead end here. I’m going to jot down here, “Not enough info about forces on the jeep to apply Newton’s Second Law to the jeep and therefore solve for T1.”

Okay, so my reaction, then, when I run into a dead end like that is to go back and reconsider my initial thought, which was to focus on Car 1. Let’s go over and look at Car 2. It also involves this tension force, T2, and therefore may be the route to our answer.

So, for Car 2, it has the same acceleration, let me draw the free body diagram for it. It also has a weight that’s balanced by the normal force. It has a pull to the right of T2. But then, as I go around the cart, I realize there’s a cable on the back end of Car 2, I’m going to call that T3.

Again, I drew it so the T3 was smaller than T2, so I end up with my net force consistent with the acceleration. Focusing again on the a(x) equation, I know my .12 meters per second squared has to be equal to plus T2 minus T3 divided by m. That’s the variable I need to solve for, I have my acceleration number, I have the mass.

Again, I’ve got another force here I don’t know. But now, looking at T3, in order to determine a value for that, I can look to Car 3 and see if that gives me a path to solving for the value of T3, and it does.

So let’s move over and work on Car 3 for a while, Car 3 is the object. It has to have, again, the .12 meters per second squared to the right acceleration. Its forces look very similar to what I’ve seen all along, the normal force balancing the force due to gravity.

As I go around this car, now the only tension forces I see that I have is T3 to the right. That gives me an equation that my .12 meters per second squared is equal to, plus T3 divided by the mass, that’s the only horizontal force that I have. And I can now solve for T3, doing a little algebra to get a number for it.

I have 39 kilograms times my .12 meters per second squared, to give me 4.68 newtons. Now, with that number I can go back. Let’s go back up here to this equation for Car 2 and plug in our, we now have a value for T3.

So let me rewrite that equation there for Car 2. It was that a(x) was equal to T2 minus T3 divided by m. Do a little algebra here to solve for the variable that we want, T2. Moving my m to the other side, I’m then going to add T3 to both sides so I have m times a(x) plus T3 now on my left. Everything is canceled on the right, so that equals T2, or T2 is equal to max plus T3 and I’m ready to solve the problem.

Let me point out that for T3, I certainly could plug in the number that I have, and that’s what most of you will do. Let me also suggest that instead of plugging in this number, I could have waited to calculate it and I, let me just plug in these variables m times a(x).

So the tension between the last car and Car 2 is only one of the car’s mass times the acceleration, but the tension between the second car and the first car, think of it as not only supporting the load of the last car, but that tension also has to provide the acceleration to the second car. They all, they both weight the same, so I end up with twice, there’s twice the tension between Car 1 and 2 compared to Car 2 and 3. That leaves me with roughly 9.36 newtons.

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