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 03 » Lecture 3, Part 4: Scalar Component Description

Lecture 3, Part 4: Scalar Component Description

https://youtu.be/PE0GwQde2qU

PHYS 1101: Lecture Three, Part Four

Now, we’re ready to talk about this notion of scalar components. It’s the last topic here before I walk you through how to add vectors by their components. The scalar components give us a really quick and useful way of just mathematically jotting down the essence, both the value and the direction of these vector components.

Here’s what I mean. I’ve got a sketch here with an x and a y-axis. My resultant vector is A, and I’ve sketched in here the y component and the x component. These two make up, are equivalent to, the sum of them is equivalent to the hypotenuse here, the resultant.

Let’s focus on one of these vector components. The vector Ay. Of course, for every vector, I need to have a way of clearly indicating the magnitude and the direction. The magnitude of that, we’ve walked through and concluded that I can get a number for that by doing my trigonometry. Off to the side here, I just draw the lengths of the sides of this right triangle. From knowing perhaps the magnitude of the vector A, the hypotenuse, I could go in and figure out the lengths of these two sides using my trigonometric functions.

The direction has to be consistent with this tail to tip direction. Ay has to capture the downward trend of vector A. But notice, because Ay, these component vectors, are always going to be parallel to the y-axis, they can either point only up or down. So mathematically, let’s associate with our magnitude a sign that can indicate for us if this vector point is actually up or down. So, we’re going to do that.

Positive in front of this would mean that this vector component points in the positive y direction. If we put a negative sign in front of it, it’s going to mean that that vector component points in the negative y direction. That’s the case for this vector. Right? It would be pointing down in the negative direction.

So, here’s what we’re going to do. When we started out the class, started out the introduction of vectors, I told you for any vector, we could describe it as having a magnitude of a certain value, let’s say in our case, 38 meters. Then, we have to include the direction information. Here, we could say it points down.

What we’re going to do now is a short hand version of this. Because this is a vector that’s always along the y-axis, I’m going to go with what’s called the scalar component description. That means I am going to write now, for my vector, my scalar component for this vector Ay, I’m going to work just with the scalar component, which is going to be just plain A with a little y subscript. I am going to write that that equals minus 38 meters.

Let me point out what is happening here with each of these components of this description. The first point here is that we call this left side of that equation, the Ay, as meaning the scalar component. The little y subscript that we have here just means this is a scalar component. It’s a part of a vector that’s along the y-axis, or parallel to the y-axis. Then, the sign that’s in front of this number tells us the direction that it points along the y-axis. Negative would be down. Positive up.

What means positive and negative? It’s going to be based on when these axes are initially drawn on your page, when you first pick or draw this initial vector, and you’ve chosen your axes, or they’re given to you in the problem. Just quick short hand. If people only draw an arrow on one end, by default, it’s assumed that that’s the positive y direction. But, it’s better to be more explicit and actually show the positive y. So, that’s what this negative here is going to represent.

Then, the last point to make is the value that you see. Let me highlight that here in blue, the number. That’s what captures our magnitude, the value we got from the trigonometry that we did. So in practice, this is what we’re going to use all the time. We’re going to take a vector, break it up into its components, and then in equations, we’re going to work with scalar components.

It’s going to have this subscript to tell us if we’re doing horizontal components or if we’re working with vertical components. The sign will mean direction, not big or small, but direction of that vector. Then, there’s going to be a magnitude or value. The kind of vector we’re working with will be indicated by the type of unit that’s associated with it.

Let me quick walk you through the mathematical picture of this or justification, because you have all the vector basics now to understand why we do this or why it’s mathematically sound to do this. Rigorously, this justification starts with defining what we’re going to call unit vectors. Small vectors that are going to point along the positive x-axis direction and one that points in the positive y. They have a length of 1.

So, at this first bullet here, let me write for you what we would originally use to describe this vector A. We would write mathematically that the vector A is equal to the sum of the vector Ax plus the vector Ay. With these unit vectors though, let me suggest to you that we can also very rigorously write that this vector A is going to be the scalar multiplication of these unit vectors. Let me write it here and then explain.

I’m going to write this vector A as having what’s called a scalar component Ax times the unit vector x-hat — this is called x-hat, by the way — plus Ay, that scalar component times this unit vector in the y direction. So, we’re just rewriting the x vector component as the product of a scalar component and a unit vector. For the y vector component, we can do the same substitution or the same thing. So, let me pull out that y description for you again. So, that means we’re focusing just on this one part to illustrate Ay. Let me just point out that in order to make this vector A consistent, this component for our particular example would end up being the vector Ay, that component vector, is equal to minus 38 meters times the unit vector ŷ.

Then, let me emphasize this for you. This vector component, Ay, we’re going to write as the scalar component times the unit vector. The scalar component, then, is going to be everything in front of this unit vector y. So, to emphasize, the sign here, that’s what tells us what direction this vector points. Negative tells us it points in the negative y direction. The number here tells us the magnitude of this vector. Then, the ŷ is just consistent with the Ay here, telling us this is a y component vector.

So, the scalar components, that’s what we’re going to work with a lot in this class. I’ve got a bullet here to emphasize that for you. This seems to cause difficulty often. There’s a tendency to want to focus on or to assign the relative size based on this sign. This negative sign here doesn’t mean that this is a small number compared to a big number. All it means is that this is a vector quantity that points in the negative axis direction. What axis? The y-axis. That will always be indicated by the subscript that you see here.

So, this bulleted statement is a good summary for you. We’re going to work with these scalar components. It’ll have a sign and a value. The variable associated with it will tell us if it’s an x scalar component or a y scalar component.

Here’s a lecture quiz question for you to see if you understand how that’s done. Given this vector, what’s the proper sign for the two scalar components for this vector, Ax and Ay?

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