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 11 » Lecture 11, Part 6: Common Forces:  Normal Force

Lecture 11, Part 6: Common Forces:  Normal Force

https://youtu.be/sLaKQ8D2X9Q

PHYS 1101: Lecture Eleven, Part Six

Next category for us to consider are those caused by surfaces. There is what’s called a normal force. This is a contribution of force that helps, that supports the load. And then there’s what’s called friction force and that’s just due to roughness that exists between this object and this surface. You always have a normal force. If any object is touching a surface, there is always going to be a normal force. Any contact, no matter how light represents some level of force.

Friction force we’re only going to see if the object is directly sliding against a surface or if there’s a tendency for the object to want to move. Imagine you could turn this surface into a slick, lick sheet of ice. If you did that, would the object start sliding? If that’s the case, you will have what’s called static friction. There is a frictional contribution from the surface that’s keeping the object from sliding. I’m going to go through each of these a little bit more carefully to give you a feel for the size and the direction.

Let’s now do the first one and talk about the normal force. This is the force that any surface is always providing simply by being in contact with that object. I need to think about the magnitude of this force which I’ll denote “F” “N” because we will use “F” sub “N”, “N” for normal and an arrow over it to represent this vector, that force. We need to think about the magnitude and the direction.

The magnitude for “F” “N” is always determined by solving Newton’s Second Law. I mean by that the same thing I meant up here for tension. It’s the value based on the “F” equals “A” “M” prediction.

In terms of direction, the critical thing to remember is that a surface can only push, never a pull. And the direction it can push is always perpendicular to that surface.

Let me do a couple of quick sketches. Let’s say we have an object sitting on a slope at this angle. We have an object sitting on a flat horizontal surface. For either scenario, because it’s contact with the surface there is a normal force on this object. The direction of it is always perpendicular to the surface. And the magnitude of it, how long this vector would be, I can only conclude the value after I have set up and algebraically solved my “A” equals “F” over “M” equations with “F” “N” as a variable.

They call it the normal force because normal is a mathematical term that means the same as perpendicular. Mathematicians say that this vector is normal to this surface.

To emphasize how the value of “F” “N” is determined I’ve got a couple of little thought experiments I want you to consider. Start out and imagine that I have on two supports something like a meter stick, kind of a long flexible stick and I put this red block or object in the middle of it. You can probably imagine pushing down on this block that a thin meter stick, a thin stick like this will be springy.

There would be the force due to gravity and then as I went around the block I would realize it’s touching this surface so I would have to have a normal force, a supporting force. That’s the only force on the object. It’s up. Surfaces can only push, so I would draw force up.

How long would I draw it? I would draw it long enough so that my visual or mathematical balance of these forces is zero because the acceleration of that block is zero. “F” net has to be zero. There’s no net up down force.

Now let’s say someone comes in and pushes down on this block. I’m sure you can imagine if I came in, somebody came in pushed down on this block, I would increase the load on this thin meter stick. It would deflect more. What does my free body diagram look like now?

Here’s my dot for the object. The force due to gravity has to be the same. I’m actually going to draw that off to the side just so slightly. It would be the exact same length it was above, looks like I drew it a little bit too long. Whatever this length is has to stay the same. In fact, let me copy this down here because that’s just the nature of this block. It’s made up of so many molecules. It has so much mass. Force due to gravity stays the same.

Now let’s go around the block. What forces do I have touching it? I still have a surface so I have a normal force. As I keep going around, now I’m in real contact with some other object, this person pushing. The person is pushing down. That’s going to be another force down.

My first pass at my free body diagram, I’m going to put sub “A” “N” “G” here for the force due to Angela. My first pass is to just get the approximate direction correctly for all of these forces. Then I start thinking about size. How big is “F” Angela? That is determined by the pressure that I would feel in my fingers at this point of contact.

If I push down harder I’m going to feel more pressure, so right at this contact point the force is larger on this object. This would get bigger and bigger or smaller so this is really set by how hard Angela pushes. Then we know that the force due to gravity is set just by the number of molecules in the block. That doesn’t change.

But as I draw this normal force, I want you to think about Question 13 to answer. Did I draw this normal force with the appropriate length? This is where you need to go back and force between our fundamental equation of Newton’s law, Newton’s Second Law. Whatever the acceleration for that object is it has to be consistent. This vector has to be visually consistent with the vector sum of these forces. “A” for the block is definitely zero. I only have vertical forces. They all have to balance.

This is fixed, the weight force, the magnitude. The force due to Angela is fixed, it’s a certain amount. What force had to get bigger is my next quiz question for you.

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