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 08 » Lecture 8, Part 6: Example – Part b

Lecture 8, Part 6: Example – Part b

https://youtu.be/xoCr00l48Zs

PHYS 1101: Lecture Eight, Part Six

Okay we have completed step 3 and we have used our trigonometry to complete as many components as we can.  Now let’s go down and make a list of our knowns and decide on what variable we need to focus on.

To make this list of our knowns, I find it useful to separate into x and y that way your eyes more easily group all the x variables together while you are looking at the x equations.  So let’s go up here and make a quick list.  I am going to do x and know that my initial position, x coordinate is zero. V0x = 13.36 m/s.  Position, velocity – I am just going to put my time here, my variable is in the middle of the coordinates of both.  I don’t know the time.

Okay so that’s at the beginning position velocity.  At the end, I don’t know the final x coordinate.  Do I know the final velocity component in the x direction?  Yes, I concluded that had to be zero if the ship was going to be headed due north.

On the other side, the y variables.  The y position initially is zero.  The initial vertical component of the velocity is plus 13.36 m/s.  That’s position, velocity at the beginning. Position at the end, I don’t know the y coordinate and the final vertical part to the velocity I also don’t know. That’s x, that’s y.

The other thing I can put between the two here is the acceleration components.  I know that Ax is -2.075 m/s^2 and Ay is +2.475 m/s^2.  Okay given these x variables and the y variables.  Let’s see if we can go after the variables that we need.

What do we want?  Let’s go back and read the problem.  First question – how long does it take to assume the original course again?  We need the variable t to answer that.  After we get that, then we need to figure out how fast it will be going.

Notice this how fast refers to the final speed – that’s going to be just the magnitude of the final velocity.  At the end, at time t and were headed due north in that instance, how long is this vector?  The magnitude of this vector is going to be the magnitude of Vy because the x is zero.  So we need t and we need Vy.  Write that here as want, we want to solve for t and Vy.

Next step, step 5 – to do this step, I went ahead and copied our equations again here to the right so we can look at them more easily. So let’s start here with t, that first question, we want the variable t, here’s a clear list of the x variables we know and of course, we have our set of x equations to use and our y variables that we know and our set of y equations.

Well t shows up in both sets, which is going to help us out.  Well my eyes immediately drawn to thinking about the x horizontal part to the motion simply because looking at these lists I know more of these quantities than I do for the y part to the motion.

Can I use this to figure out the time?  Well let’s see time shows up in this very first equation.  Final horizontal velocity is equal to the initial plus Ax*t.  I have Ax, I have the initial horizontal velocity, the final – that equation would work for me, I am going to use that one.  I am going to use Vx = V0x + ax where I know all three of those quantities so if I do all my algebra, I subtract that to the other side and divide by Ax.  Check my algebra in more detail if you need to.  t = Vx – V0x/Ax.

Plug in numbers for that, my final Vx is 0.  So I have that t = 0 – 13.36 m/s / Ax which is -2.475 m/s^2.  Quick unit check, I am feeling good, the meters cancel in the numerator and dominator.  One of those seconds cancels with one of those seconds.  The second in this dominator in the dominator is going to go up to the numerator.

Also notice that by carefully keeping track of the signs, the correct sign values here ended up in a negative and a negative cancelling so time is positive which is good.  That’s what you would physically, physically make sense.  I end up with t = 13.36/2.47 that is 5.398.  Keeping four digits that’s a little over 5 seconds, I would actually type into WebAssign 3 digits and I would round to that 5.398, the 8 would round this up and that would make this 40.

The next thing we needed to know was the final speed, the final speed the magnitude of the final velocity.  That’s how fast it would be going at that instance.  And you remember our final velocity was a vector pointing straight up which means it only has a y component so what we really need to focus on is the variable Vy as I said here.

So let’s look at our y equations and our list of y variables and see what we know, what will get it for us.  Let’s look at this first equation, that’s looking really good to me.  I want Vy, I do know what the initial vertical velocity is, I know Ay, and I know now t.  I can use that equation directly. T is now a known value.  If it took long for the horizontal velocity to go back to zero and in that same time, I can calculate what happened to the vertical part of the velocity.

So I am going to use equation one of the y equations.  Vy = v0y + Ay*t.  I can just plug in numbers directly for that.  V0y was +13.36 m/s plus the vertical component of my acceleration was +2.475 * time and my time is – I’m going to plug in the full four digits for that because then at the end for this final answer, I am just going to grab the three digits.  I am going to put in 5.398 s.

Let’s do a quick unit check.  This second cancels with one of those so I am left with m/s.  That does make sense to add to a quantity that is m/s and of course, that’s the units I am looking for.

When I plug this into my calculator, I get 26.7 m/s rounding to my three digits.  So my two answers are it takes 5.40 seconds for that boat to get going due north again and after it’s done that, its headed due north with a y component to its velocity or its velocity vector having a magnitude of 26.7 up – that is the speed, that is how fast it is going so that is what I would type in.

So you notice this is quite a bit bigger than the initial velocity that I had. Does that make sense? Quick let me go back to our picture here, let’s see if it makes sense.  My acceleration in this direction, it does have this negative x component to it, so that’s going to decrease the horizontal velocity and bring it to zero. At the same time it has a vertical acceleration component here – that’s going to cause the vertical part of this velocity during the same time interval to just keep getting larger and larger by that delta-v. So I probably didn’t exaggerate it enough, that this final velocity is actually quite a bit bigger. It is roughly double than what this initial height was. That’s a little overboard now.  It looks like that.

So that’s a good picture of velocities at the two snapshots giving this acceleration of what our ship does to this problem.  So for this last point here, the last step to think through and make sure your numbers make sense, I went back and looked at the acceleration vectors and velocities, checked our units along the way, as best as we could tell it does look all and good. It does make sense.

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