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 7: Scalar Addition Example

Lecture 3, Part 7: Scalar Addition Example

https://youtu.be/e-L1memZH1w

PHYS 1101: Lecture Three, Part Seven

Okay. Let’s do an example. Let’s say we’re given these vectors, A and B, and we want to know what the magnitude is. First, we’re going to start out, do step one here, and then we’re going to find the scalar components. I’m going to copy vector A on the left. I’m going to copy vector B on the right, and I’m going to set up here to do my trig.

For vector A, I’m sketching in the two sides of this triangle. There’s Ax. There’s Ay. And here’s Ax. Let me do that in blue. Okay. So, that shows me the direction, and that will indicate the proper sign I need for these vectors, but I’m going to do my trigonometry just to get the values.

Let me sketch the triangle real quick again here, off to the side. The hypotenuse is 3. I have 45 degrees, and here is the sides Ay and Ax. So, Ax is going to be the hypotenuse, 3 times the cosine of 45 degrees. That’s 2.12. Ay is going to be 3 times the sine of 45 degrees. That’s also equal to 2.12.

Now, let me go off to the side of each of these and be sure I have the sign correct for the real scalar component. Ax, I actually need to make negative because the Ax vector component points to the left. So, that’s -2.12. Ay, the y component vector points up. That is in the positive y direction, based on my axes here that you see. So, Ay is going to stay the same, positive 2.12.

Okay. Let’s go take care of this for our B vector. I’m going to sketch my right triangle here, off to the right. Here’s going to be my y vector component, and here’s my x. This is the vector By. Here’s the vector Bx. So, now these arrow directions here will help me pick the right sign.

If I do my trigonometry, I know, let’s see, if this is 56 degrees, this has to be 90 degrees minus 56. That’s 34 degrees. So, I’ll go ahead. I have to get an angle, one of the angles inside of my right triangle, in order to do my trigonometry. So, I just had a tendency to want to go after this angle. So, given that 34 degrees, the hypotenuse is 6.5. I’m now set to get the lengths of the two sides.

Bx, that’s the opposite side to this angle, so it’s going to be 6.5 times the sine of 34 degrees. That is 3.6. Let me do my little arrow here. What’s the proper sign for this component? It has a magnitude of 3.6, but it does point to the negative x direction. So, I’m going to write that Bx is -3.6.

By, that involves the adjacent side to the angle that I have, so that’s my hypotenuse. 6.5 times the cosine of 34 degrees. The number I get for that is 5.4. Now, the real scalar component, after I carefully assign the proper sign to this By scalar component, I’m going to end up with -5.4. That vector points down.

I have my scalar components now. I’m ready to make my table. So, here I go. I’m going to do x and y. I’m going to do vector A plus vector B, is going to give me vector, we’ll call it “R”, the same resultant. Now, I just need to fill in my values from the table, the values from above, fill in my table.

So, let’s do for vector A. My x component is -2.12. My y component is +2.12. For Bx, I had -3.16. And y, I had -5.4. Now, I’m ready to just add down these columns. This means that my resultant for the x component is the sum of these two. That’s going to be -5.72. My y component is going to be the sum of those, which is going to be negative 3.28.

Let me emphasize again, this is the x scalar component of my resultant, and this is the y scalar component of my resultant. So, that means I can write off to the side here that my vector R is equal to -5.72 for its x scalar component, plus -3.28 for the ŷ unit vector. So, that’s my y scalar component. There’s the x, and there’s the y. So, that’s one way of writing this vector R.

Now, let’s go in and get the magnitude, as we were asked to do. I’m going to, real quick here, draw a sketch to be sure that my scalar values seem to make sense. But to do that, just to make it easier, I’m going to go up here and copy these vectors again. Let me paste them right here. Let me go in and just clean them up a bit here.

There’s vector A. Here’s vector A. Vector A plus vector B, the tail to tip sum would be from the initial tail out to the final tip. This is our vector R. And reminding you that our axes directions that we picked were the standard plus y up, plus x to the right. So, that means if I focus just on R, our resultant, and think of breaking it up into its components, I would expect to see a vector Ry that points down, and a vector Rx that points to the left. Ry, the scalar form of that should be a negative number, and Rx, the scalar component should also be a negative number.

And you know what? That’s consistent with what we found. Notice the relative size of these two is also consistent. The y scalar component is negative, but it’s a smaller magnitude than x, and that matches our picture.

So, what’s the magnitude of R? I just want to focus on the lengths of these two sides and use my Pythagorean to figure out the length of the hypotenuse here. So, I would write that my magnitude R is going to be the square root of just the lengths of the sides. So, here I don’t need to worry about the sine. I have Rx, which I’m just going to use 5.72, positive number squared plus my Ry squared, 3.28. Again, the sign just represents direction here. When I’m after the magnitude, I’m just doing geometry again. I’m comparing the lengths of the sides of this triangle, where for just this exercise, I’m not worried about directions. So, I can forget about the sign that conveys direction. When I multiply that out, I get 6.6.

Now, let’s say I wanted an angle. Just follow through here. I’ve redrawn it here, re-sketched it. Let’s say I want to go after this angle,

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