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 05 » Lecture 5, Part 06: Example 2

Lecture 5, Part 06: Example 2

https://youtu.be/4U_-H6LT8Qc

PHYS 1101: Lecture Five, Part Six

Here we have a sports car picking up speed. It passes between two markers in a time of 4.1 seconds. The markers are separated by 120 meters. All the while, the car is accelerating by 1.8 meters per second squared. What is its speed at the second marker?

Here are steps. Visualize, what object? It’s going to be the sports car. Start to end. The start to end would be this passing between the two markers. Marker 1 is going to be the start and marker 2 would be the end.

What does the motion diagram look like? Let me sketch that above here. First here is my car, and that’s such a well-drawn car. I’m going to copy it over here at my finish. I’m sure you’d agree. The motion diagram now. Is this car starting from rest at the first marker and speeding up? Can I make that assumption? I don’t think I can. It says that the car is picking up speed as it passes between the two markers. I think it’s already going at some initial velocity and it’s then the velocity is definitely increasing, but that it has some initial velocity. I think I have to draw this for the motion diagram. My acceleration vector, just for reference, it’s acceleration, it’s increasing speed, same direction.

That’s a good initial picture of the scope of my problem. Now let’s be more specific and follow step two and find an axis and an origin and start thinking about our variables. The convention we picked for the previous problem would work well again here. So here I’m going to put my origin at the first marker. Here’s my second marker. Here’s my object we sketched at these two instances.

Okay, draw an initial velocity vector and draw the final just so you solidify in your mind whether they’re 0 or not, if they’re getting smaller or bigger. I will go ahead and draw an initial and a final. Because I’m near the edge of the page here I’m going to move that over a little bit, and I’m going to make my next and last velocity vector clearly bigger.

Think about these variables: time, position and velocity at each of these instances. Start my clock at 0 as usual. My initial origin. My origin is where the object is at that initial instance, so it’s positioned at 0. Do I know its initial velocity? I don’t. It’s positive, but I don’t know a number for it. Time, position and velocity at the end.

Time to cross the second marker, it looks like I do know that. It took 4.1 seconds. What’s its position coordinate at this instant given this is our origin? It looks to me like it’s going to be at the x-coordinate of +120 meters.

Then do we know our final velocity, the velocity at this instant? No we don’t. In fact, that’s what we need to know. This is what we want. If we get this final velocity, we know that the magnitude of that, just the positive value will be the speed and that’s what we have to type in, just a positive number meters per second for our answer.

The last variable to consider is a. Do we know what the constant acceleration is between the start and the finish, the two markers? You know what, we do. It’s 1.8 meters per second squared.

Okay. The next step here is to make our list of knowns and the variable we solved for. In fact, it would be a little bit redundant to repeat that entirely. Well, I don’t want to copy it. I’m just going to move it down a little bit and note that this really is what we’ve done by jotting down these quantities as we thought through setting up our problem. I am going to focus, though, or help me to focus by clearly saying that the variable I want is v, the final velocity.

Next step, pick equations and algebra our way to a solution. Let me go grab again a copy of our equations, our starting equation. All right, here they are. The first thing I’m going to do is go in and highlight the variable I want, v. Here it is, and here it is.

Next thing, I’m going to highlight the variables that we know and that we have. Do we know v0? No. Do we know a? Yes. And we know t. We know a and t. We know the position coordinates at the beginning and the end. It looks like that’s it. The variables that are not highlighted I don’t know and I need to solve for v.

My eye is really drawn to using this one, but I don’t know the initial velocity. You know what, I need that initial velocity for any of these equations. Here’s a strategy. What do you think of this idea? I don’t know the initial velocity but you know what? If I were to solve for the initial velocity and substitute it in, say, to this equation or this one, I would then remove that initial velocity from my equation. Let me just show you what I mean.

Let’s take equation one. Let me just write here, strategy. This is where there is no necessarily right or wrong answer. There are different ways to solve this problem. You just have to be sure whatever direction you head, you always mathematically do legitimate steps and you may find you head in a direction that doesn’t get you anywhere and you need to go back to the beginning and try a different strategy.

I’m just first going to start out thinking about equation one and realize that I don’t have any information about v0. For me to use any of the other equations, I really need to get rid of this variable v0. So let’s solve for v0 and then use this to get rid of v0 in another equation.

How do I? Let’s solve this for v0. In order to do that I’m going to subtract at from both sides. I’m going to end up with v minus at is equal to v0 plus at minus at, which is how I’ve moved it over to the left hand side. So if I just rewrite that as I would read it, v0 then equals v minus at. By solving for v0 now, I know I can replace v0 anywhere with its equivalent, what shows up here on the right hand side. These are all variables for which I have numbers for, so by substituting this into, let’s say, this equation, I will have gotten rid of this variable I don’t know.

I’m going to put here sub into equation two. You could have as easily substituted into equation three if you wanted. My eye is drawn to two. Let’s first start with equation two and I want to remove any terms that are 0 just so my algebra . . . it looks a little simpler in my equation that I’m working with. Let’s see, my initial marker and therefore my initial coordinate was 0. Looks like that’s the only one I can get rid of. x is equal to v0t plus one-half at2.

Now I’m going to do my substitution. We can move our next problem down. So for v0 I’m going to substitute in v minus at. x then is equal to v minus at, that’s for this. I still have to multiply by t, and then I have to add one-half at2.

I’m after the variable v, meaning I need to rearrange this so I have v is equal to blah, blah, blah, variables for which I have values for.  So I need to do some algebra here. In order to isolate v I first have to multiply in this t. vt minus at2 plus one-half at2. I have to, in order to isolate it, I need to get v related to the other variables in terms of a sum or a difference so I can start adding and moving them over to the other side.

Well, I recognize that this is the same variables as this, so I can add these two quantities together. Here I have minus 1. If it’s not written there, we know explicitly that it’s 1. Here’s plus one-half. So minus 1 plus one-half is minus one-half. So this is also equal to minus one-half at2.

Now I’m going to move this over to the other side and end up with having canceled the terms on the left. The other step I can do now is divide by t. Of course I have to divide the whole side, right and left, by t. That cancels out  that variable and so then on the right I have v now is equal to one-half at2 plus x, all divided by t.

Now I’m ready to actually plug in numbers. Let me just flip the order of that so it more naturally reads left to right. v is equal to one-half at2, that’s fine to switch this order, divided by t. So this equation is now mathematically consistent with our initial equations but now we have used the mathematics to convert it into a form that gives us our answer directly.

The v that we’re after now is equal to the final position. I have to add the product of one-half acceleration times time squared and then divide that sum by the time and that number will give me my final velocity.  Let’s plug in the numbers and see what we get. Our final x-coordinate was plus 120 meters and then I have to add one-half times a, 1.8 meters per second squared, times our time squared. That was 4.1 seconds, and then I have to divide this by the time, 4.1 seconds.

Let me look at the units here real quick before I punch that into my calculator. We learned before the second squared here cancels with the 2 seconds I have in the numerator there and I end up with meters being added to meters, good sign. I’m going to end up with meters in the numerator divided by seconds in the denominator, a second excellent sign. v does have units of meters per second. So far so good. Let’s get a number for it, see if it makes sense.

I end up with the final velocity as being plus 32.96 meters per second. I would round that to three digits. 6 rounds us up and I would write 33.0 meters per second. That is how I would type it in.

Let’s see if this physically makes sense. Let me go back up here and just grab our last step because that’s what we’re doing now. Just a quick check. We’ve already checked the units, so our algebra is good. We might have plugged it into our calculator incorrectly. Let’s see if it physically makes sense.

Rule of thumb, to get from meters per second into miles per hour, which is more intuitive to us, you just roughly multiply by 2. So 33 meters per second is roughly 66 miles per hour. Let’s think about what the initial velocity was. Oh, you know what? We never got a number for that so I just don’t know.

We could go back if we wanted. Here, for example, we could use this equation, plug in our 33 meters per second using the a and the t. Actually, I would plug it into this equation. The initial velocity would be 33 minus 1.8 times 4.1 seconds. In fact, I’m going to do that calculation right now in real-time for you. 4.1, multiply these together and then I’m going to . . . I get 25.

So the initial velocity was about 26 meters per second, so that’s about 50 miles per hour. So this car appears to be going 50 when it passes the first marker and with this acceleration of roughly 1.8 meters per second squared, by the time they cross the second marker they’re going about 66 miles per hour. Seems reasonable. That’s as much as I would check to see if the answer seemed reasonable. So I’ll just put a little check mark there. Seems okay.

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