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 5: What is a Force?

Lecture 10, Part 5: What is a Force?

https://youtu.be/V_9jvFmyj3A

PHYS 1101: Lecture Ten, Part Five

So here are my criteria that I want you to continue to go back to as you try to fine tune your identification of forces on objects because to get the motion correct, understand it properly, you have to be able to identify, and you have to know what all the forces are on an object. Every single force has to be a push or a pull on that object. And it’s always a single object that we’re going to focus on at a time. That push or pull on that object always is going to occur at a very specific contact point on that object.

It will be because some agent, a person, a table, something that’s touching that object is making contact at that point. It doesn’t matter how light that contact is or how strong, there’s a force there. The size of the force depends on how light that touch is or how strong it is. But any contact, you’ve got a force. Force, as you can appreciate from this definition, I think, has both a value and a direction that are important. It’s a vector.

Mathematically, that’s how we’re going to have to treat it. The second bullet down here emphasizes what I pointed out before is that for every force, there’s always an agent or something that’s directly responsible for that force. If you ask yourself, every force that you’re wanting to draw on an object, what the agent is, it can help you catch yourself making a mistake of improperly identifying a force. That agent, it can be animate or inanimate.

My laptop is sitting on this table, and from the laptop’s perspective, it feels it’s in contact with the table. That table is exerting a real force on the bottom of that laptop. If I were to pick up and hold my laptop, I would feel the contact with that laptop so that laptop would be experiencing the same force of support from my hand as it did from the table.

So that’s a case where I have the same force, but you’re seeing it could be due to something animate, like me, or inanimate, like the table. We’re going to work with forces in a lot of our equations. We want to be sure we understand what the equation is, and I’m going to get to that in a minute. Here I want to remind you, or point out that a force is always in units of a Newton. That’s the SI unit for force. And one Newton is equivalent to one kilogram times a meter per second squared.

To give you some physical intuition of what one Newton means, if you were to put a small apple in your hand, your hand would have the sensation of a gentle, downward push from the weight of that apple. The size of that push, that’s about one Newton. So we get to problems, and it says there’s a hundred Newton force on something, you can picture a hundred apples. What does that feel like? That’s what that object is experiencing.

Okay, question eight for your quiz. Let’s see if you can put this together. I show you different motion diagrams, and I want to ask which of these objects is experiencing a net force? And what I’ve argued above is that if I have a net force, that means I have to have a change in velocity. Which of those motion diagrams satisfies that criteria? Which of them is showing acceleration?

Question nine asks you the same thing, but now in the context of a mixture of one-dimensional motion versus trajectories, curved motion, curved paths in two dimensions. Which of these motion diagrams similarly represents a net force? Again, the net force means I have real delta v velocity vectors, which we know means I have acceleration because the definition of acceleration is this delta v vector, the change in the velocity vector divided by time.

I have another question for you to get you to look at it in a slightly different way. Again, it’s just putting pieces together that you know from previous work and applying it to what I’m teaching you now.

Question 10. This motion diagram below shows you that definitely the velocity is changing. This object goes from one to two to three to four, etc. You see the time sequence. What arrow best represents the direction of the net force on the object at instant three?

From net force, I hope you’re making the connection that you need to then be thinking about or asking what’s the acceleration, or what’s the delta v? Where? At instant three. At instant three, what’s the change in velocity? Here’s my summary for you of identifying forces. The first comment I’m going to make is that every single force in this class… This class deals… It’s mechanics. It deals with the motion of day-to-day objects.

Every force, it has to be a contact force. Something is directly touching this object. Pulling on it or pushing on it. There’s only one exception, and that’s the force due to gravity. And we’re going to use w, where the w represents the weight of the object to represent that force. Gravity, with a handful of other forces, is what’s called a long-range force. Meaning, there doesn’t have to be direct contact for this force to exist.

Another example of a long-range force is the magnetic force. If you take two magnets… I’m sure you’ve all experienced this. If you put opposite poles together, they don’t have to be touching for you to feel that there’s a pull between the two. If you change the orientation, and you try to push two poles together that are the same, you’ll feel this push away from each other. Magnetism is another long-range force.

You’ll deal with that in 1102. In 1101, we only have one long-range force, gravity, and it’s somewhat counter-intuitive because none of us have the experience of not experiencing the force of gravity. It’s always there. It’s on every object that we see. It’s on us all the time. So aside from gravity, you just have to then identify the rest of the forces on the object. And all of them have to be from something that’s really in contact with that object.

The gravity force, a few more bullets here point out, the size and the direction, the two questions we have to ask about every vector. How big is it? The magnitude will be the mass of this object times 9.8 meters per second squared. And the direction? The force due to gravity is always straight down. It’s actually pointing straight to the center of the Earth, and from all of our perspective, that just means straight down.

So here are your steps for identifying forces. Use red. Use a specific color pencil, if you’d like, to really hone in on and identify the single object that you’re working with for your problem. Immediately draw a blue arrow down and label it w to represent the force due to gravity. Next, imagine drawing a circle around this object.

Let’s give ourselves an object here so I can illustrate. Here’s my object. It’s some person that’s described in some problem. I’m immediately going to go draw my force due to gravity on that object and label it. Then by step two, I’m saying, “Imagine a hypothetical circle around this object.” Let’s say that in reality this object, we are told, is standing on the ground and maybe is pulling on a rope.

With this imaginary circle that you’ve drawn, start somewhere. Start here at 3 o’clock. Go around clockwise if you want, and be very rigorous as you go around. Any surface that breaks this circle and is making contact with that object, there’s a force at that point. There’s contact there.

So on the ground, we’re going to learn that the ground in truth pushes up on the object. And then, once we’ve got the ground considered, I’m going to keep going around. Nothing’s breaking the circle here. Nothing. Nothing. There’s a rope that’s breaking the circle. That rope is in contact with this person. So I’m going to add another force to represent the tension in that rope.

What these forces, what direction, how big they would be, that’s what we’re going to continue to work on as we go through the next three lectures. What’s critical is that you have to be rigorous to get all forces. If you don’t get them all, then Newton’s second law will let you down. The mathematics won’t properly predict what the acceleration is because it has to be the result of all the forces on some object that lead to some net force or don’t, which then sets the acceleration, which then sets the trajectory for this object.

If we were in a classroom, and I were lecturing to you live, I would at this point show you a real demonstration of shooting a ball straight up into the air. For an online class, the best I can do is show you this animation. So pretend this is a cannon. There’s a spring under here that gives an initial kick to this ball and shoots it straight up into the air. So pretend you’re watching this in real time.

As you watch that movie, I’m going to ask you quiz question number 11. Now if you want, focus on the upward part of this motion. When that ball is on its way up, what list best describes the forces that are acting on it? This is very important question as suggested by the point value that I’m going to give it. I’ll give you eight points if you get this one right.

When that ball is on its way up, choice A is there a force of gravity and the force of this plunger or spring on the ball? Is there B, just the force of gravity? Or C, just the force of the plunger? To answer that question, take the time, and go back, and follow these steps. Follow this advice to help guide you to be sure that your first, intuitive feeling for that question is right. Now, I’ve given you a physical intuition, or I hope I have, for what Newton’s laws, his first and his second law, are.

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