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 10 » Lecture 10, Part 3: Dynamics:  Why Does Velocity Change?

Lecture 10, Part 3: Dynamics:  Why Does Velocity Change?

https://youtu.be/Fc9CoR5im_4

PHYS 1101: Lecture Ten, Part Three

Chapter 4 is the step beyond just describing motion. And it’s what we call dynamics. It’s the categorization effectively asking the question, “How or why do velocities change?” You’ll see why that’s the fundamental question behind dynamics here in a minute.

I’d like to begin this discussion with the first step of asking you to consider what’s your intuition? What do you think is the natural state of an object? And by natural state, I mean, if you left this object alone, if nothing is touching it, nothing is done to it . . . What’s its natural state? What would happen to the motion? What’s the natural state of the motion that would result?

For question 4, I’ll give everyone 3 points for just giving me your opinion? What does your intuition, coming into this class, tell you the answer to that question is? Is the natural state, in terms of the motion for an object, to A) come to rest, to keep meeting, or do you think it just depends on the situation?

To try to ease ourselves into thinking about this more critically, I’d like you to do this demonstration. Likely you have something in front of you that you could use to do this. Imagine, or let’s picture you have a book in front of you on the table that you’re sitting at. Try giving this book a push. Give it a quick push, let go. Give it enough of a push that you actually watch it slide for a bit before it comes to a stop.

With that kind of motion, and then thinking about this question: What’s the natural state of an object?

For 3 points, give me your opinion for question 5. Ask yourself, after the push is done, after you’ve let go, why does the book keep moving forward? Is that A) because of the force behind it coming from the push? Is that B) because it was given an initial speed from the push? Or C) Neither sounds quite right.

This question focuses on why does the book keep moving. Let’s ask it from the other perspective, which is why does the book slow down? What’s your opinion when you think about it from that side? What causes the book to slow down? Is it A) friction eventually overcomes the force of the push? Does that sound right to you? B) Friction alone slows it down or C) Neither sounds quite right.

Enter your, your intuition, your perspective. I’m not going to grade that. I’m just going to give everyone 3 points. Though, let me now say a few words about what the right answers are to these. But, historically, what people believed and what they struggled with coming to accept the right view.

It turns out that at the time of, say, Aristotle, or even much later, the scientists in the medieval period. They had this perception of what is called an Impetus Theory, meaning that when an object was pushed, there was some impetus that was imparted into that object. And that’s what caused it to continue to move forward. But then, different versions described what happened somewhat differently. But in essence, the picture was that this, this impetus gradually leaked away or went away, if you will, and that’s why the object came to a stop.

So in blue, I’ll highlight that many great minds in history and in the past likely would have chosen A. They would have said that that book keeps moving forward because of the force behind it coming from the push.

Newton quite revolutionized our view of motion, which is the whole heart of this class. Newton proposed that, well, the reason the book keeps moving forward is just because it was given an initial velocity from the push. That’s all it took. It no longer needs a force for it to keep moving forward.

So let me do here, and note that this is the old view. Studies show that the majority of students coming into a physics class, your typical person on the street, will, will have some form of this view. B is what Newton tells us. Newton’s view.

Okay. From the perspective of why does the book slow down, along the same lines, somebody like Aristotle would’ve answered something like, “The book slows down eventually because there’s roughness from the table, or what we now call friction, that eventually overcomes the force of the push.”

Newton, though, argued that you could just as well explain the motion by noting, or invoking, the idea that friction alone is slowing the book down. So, from the motion diagram picture, Newton might jot down, “Here starts out my book. It slows down, comes to a stop. And we now know in terms of our building blocks to describe that as a velocity that’s decreasing. And, therefore, an acceleration that points in the opposite direction.”

And Newton would argue all that book needed was an initial velocity and some single force that opposes that motion that causes this book to slow down. And translating that to our building blocks, that means a constant force causes this Delta v or the deceleration of that book. So, again. Over here, let me highlight for you. This is Newton’s view . . . And this is the old view . . . And I suspect that if many of you kept with your initial answer, your first intuition, that many of you quite naturally, and in good company, would have chosen A perhaps for both of those questions. So, much all of chapter 4 is getting you to appreciate the concepts behind these choices B.

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