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 8: Your Turn

Lecture 13, Part 8: Your Turn

https://youtu.be/vgFw-wCIGSo

PHYS 1101: Lecture Thirteen, Part Eight

The next example has you putting these ideas together from the previous examples that I’ve done. You have a tilted coordinate system to work with, very similar numbers to what you had above, a 10-kilogram mass on a slope. I’ve changed the angle of the slope. And you need to, then, evaluate the motion of this block. Not, now, it’s no longer on its own sitting on the surface, but there’s a rope attached to it that goes over a pulley and is attached to this 3-kilogram block hanging at the other end.

There’s a whole series of quiz questions now that ask you about different aspects of that to help you solve this problem. Ultimately, you’re going to be typing in the value of the acceleration of the block along the slope.

When you’re faced with a scenario like this where you don’t immediately know for sure what direction it’s going to move, is this block going to accelerate down the slope or up the slope? This scenario, each scenario would be possible depending on the angle of the slope and these masses.

I advise that you pick one and then be consistent with that. When you get a number for your acceleration; if it turns out to have the opposite sine to what you thought, then it would tell you that it’s the other scenario that’s happening, given the masses and the angle.

So, let me start you off by assuming you have a motion diagram for the block along the slope that looks like that. That says that the force due to gravity or the part of it along the slope for this 10-kilogram block overcomes the tension in the line trying to keep it from sliding down the hill. Therefore, the acceleration is in that direction. Assume that and work with it as you work the problems.

Regardless of this assumption, you still can consider how the accelerations compare. That is, the acceleration of block two compared to the magnitude of the acceleration of block one. That’s question 15.

Question 16 is asking you about the direction of the acceleration vector for these blocks. Go with the assumption that I noted at the top. For block one, what arrow best represents the direction of its acceleration? Everyone should get this right. That’s question 16.

Question 17 is going to be what arrow best represents the direction of the acceleration for block two? For question 18, what’s the best coordinate system to use to evaluate our f equals ma problem for mass one?

Remember, you can pick the coordinate system that you want for each object and they don’t have to be aligned the same; they can be separate. The only thing you have to be sensitive to is be sure that you connect the accelerations properly given those two coordinate systems. And that likewise, the direction of Third Law pair forces get assigned properly, based on the coordinate systems. So, for mass one along the slope, what’s the best coordinate system to use? Everyone should get this right.

Question 19, this is for block mass 2. What’s the best coordinate system to use to apply the problem solving steps to the mass hanging off the end of the ramp? And if you’d like, do it as I do where I separate it on the page. On the left side of the page, I’m going to write out my problem solving steps, applying Newton’s Second Law to block one. On the right side of the page, I’m going to write them out for block two.

And that’s what my subscripts here indicate. For block two, the one hanging off to the left, how will the acceleration direction, the scalar components compare? Let’s assume you go with the typical convention with positive being up for the block off to the left. Which of these is right?

Question 21, what’s the magnitude of the component of the gravitational force for block 1 that’s along the slope? What’s the magnitude of the gravitational component that’s perpendicular to the slope?

Question 23, calculate the value of the normal force on block 1.

Twenty-four, enter the number for the magnitude of the friction force on block one. You have the same coefficient of kinetic friction of 0.1 for the scenario.

Question 25, how large is the tension in the rope? And then, last, you should have all the pieces that you need to put it together, then, for what’s the magnitude of the acceleration?

And then, I’m going to end the lecture with a bonus point opportunity for exam two. We’re still going to have our sample exam where you can earn bonus points, which is a copy of last semester’s exam two. But in addition to that, you can earn two extra points if you can correctly solve this problem that I laid out at the very beginning of the lecture to motivate Newton’s Third Law.

What is the tension that you need in this rope in order for the blue block to accelerate to the right at 4 meters per second squared? You should have enough tools, now, to be able to solve that and this is about as complicated as it gets. You have to take it slowly and just break it down.

Again, the strategy I might use, it’s a lot like what I pointed out here at the end of question 26. This quantity that you’re after, you know it’s going to show up. It is one of the forces on block one. Therefore, you really want to start with the a(x) is equal to the sum of the horizontal forces divided by m for the purple block. Start there.

This variable will be in this equation, but you’ll discover that there are other force values that you don’t know that you need a value for. And that’s then, what’s going to have you focusing on equations involving this block to solve that. So, keep breaking it down, keep going after the pieces that you need in order for this equation to give you the value of T1.

Okay, work that out. Send me your answer, three digits is fine. Send it to adavies@uncc.edu. That’s the end of lecture 13.

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