Monday, December 8, 2014

Unit 3



A. Newton’s 3rd Law and  Action/Reaction Pairs

  • Newton's third law states that every action has an equal and opposite reaction
  • For example, when you walk, you push the ground back and the ground pushes you forward
    • The difference is that the ground has a much greater mass so its acceleration is much less
  • Another example is if you push someone in a chair 
    • You push the chair and the chair pushes back on you
    • The reason you don't move is because you push the ground forward and it pushes you backwards
      • This is similar to the tug of war/horse and buggy
  • Even if nothing is in motion forces are still in action
    • If a book sits on a table the book is pushing the table down and the table is pushing the apple up
    • The book is always being pulled down by the Earth and the apple pulls the Earth up
B. Tug of war/horse and buggy


  • Many people are under the impression that to win a tug of war battle you must pull the hardest
  • This is false
  • We know that from Newton's Third Law every interaction there is an equal and opposite reaction
  • This means that pulling the rope harder just means the other team pulls just as hard
  • The truth is that winning is not based on how hard you pull
    • Rather it is based on how hard you push the ground
  • The person who pushes the ground the hardest will have the ground push them back the hardest, therefore the winner is whoever pushes the ground the hardest
C. Forces in perpendicular directions

  • This is best described by a box sliding down a ramp
  • The weight of the box is caused by gravity and will always be in the downward direction
  • The box pushes up while the ramp pushes down
  • When drawn the vectors will end up in the diagonal direction causing the box to accelerate down the ramp
  • The steeper the box, the greater the acceleration the box will have
  • This can also be seen in someone canoeing across a current going downstream
  • If there is a velocity going down stream and a velocity across the velocity will end up being in the diaganol direction and the person will not canoe straight across
D. Gravity and Tides

  • The force of gravity is increased as the mass of the object increases

    • The more mass an object has, the more it is attracted to other object
  • The force of gravity is defined by the formula: 
  • As mass goes up so does the force
    • They are directly proportional 
  • As distance goes up, the force goes down
    • They are inversely proportional
  • This is why the moon has a larger impact on the tides than the sun does
    • Though the sun's mass is much greater than that of the moon's,the moon is much closer
    • When mass goes up by the same factor that distance does, distance  has the greater impact
    • If mass goes up by a factor of 2, the force doubles
    • If distance goes up by a factor of two. the force goes down to 1/4 of the original force
    • The reason why distance has a greater affect is because it is squared
  • The tides of the Earth are most affected by the moon
  • The force of the moon on one side, and the much less force it has on the other side of the Earth is what causes what is called the tidal bulge
  • The tidal bulge is caused by the moon pulling on side very hard, and very weak on the other side, because they have a greater distance
  • The moon pulls one side hard, the Earth comes over some and then the oceans are spread thin causing the North and South side to have lower 
  • When the moon is on the East side of the Earth, the oceans on the East and West side will be in high tide, and the North and South side will be in low tide
E. Momentum – and Impulse momentum relationship

  • Momentum is a way to describe an object in motion and with relation to the object's mass
  • If two objects are in motion with the same velocity but one with a higher mass, the one with the higher mass will have the higher momentum
  • Momentum is also p
  • p=mv
  • When an object's momentum changes over a period of time, it is called an impulse
  • Impulse is also equivalent to the change in momentum
  • Impulse is J\
  • J is also to be calculated 
  • Impulse is what determines how you hit the airbags 
    • Regardless of how you hit the airbags you will go from moving to not moving
    • The airbags increase the time but impulse will not change
    • The airbags therefore decrease the F
    • The impulse of you hitting the airbags versus hitting the dashboard are the same because the change in momentum is the same:moving to at rest
F. Conservation of Momentum (Including the lab)
  • Within a system we know that momentum is conserved
  • For example, if a 5kg cart is moving at 6m/s and it hits a 1kg cart and stops, it has to have the same momentum as the other cart
      • It will be moving at 30m/s
      • This can also be solved by using M(a)V(a)+ M(b)V(b)= M(a)V(a)+M(b)V(b)
        • 5(6)+1(0)=5(0)+1(x)
        • 30+0=0+x
        • 30=x
    • If the objects stick together then you must use another formula such as M(a)V(a)+M(b)V(b)=M(a+b)V(ab)
      • The ab at the end are not to be multiplied but is to show that the two objects are now one and stick together
    • If the objects in the previous stuck together rather than the first one stopping it would be 5(6)+1(0)=6x
    • 30+0=6x
    • 30=6x
    • x=5m/s

    Monday, November 17, 2014

    Tides Resource Post

    This resource was very useful because of the in depth explanation of each part of tides. He explains the different types of tides (spring and neap), and also depicts when each of them occur. Many animations were used to explain the tides as well as why we have the tidal bulge.  Tides occur because the moon pulls the ocean up towards it and the ocean is then spread thinner causing low tides in the middle, and since Earth is pulled up by the moon also there is high tide on the opposite side. Tides are caused because there is a difference in forces on each side of the Earth. Tides change every 6 hours, so there will be 2 high tides and 2 low tides per day. Tides are very dependent on the moons and its alignment with the sun. When all three of us are lined up, we get spring tides, causing higher high tides and low low tides. On the other hand a neap tide is when we form a ninety degree angle and the sun negates some of the moon's pull on the ocean. This causes low high tides and high low tides. Right now on Fripp Island in South Carolina, they are experiencing a high tide, but in an hour it will be low tide. The moon is approaching a new moon and is currently in its last quarter. 

    November 2014

    DayHigh

    Low
    High

    Low
    High
    PhaseSunriseSunsetMoonriseMoonset
    Sat 0103:10 AM EDT 6.48 ft09:23 AM EDT 0.61 ft03:44 PM EDT 6.85 ft10:05 PM EDT 0.34 ft07:38 AM EDT06:31 PM EDT03:05 PM EDT01:52 AM EDT
    Sun 0203:11 AM EST 6.77 ft09:29 AM EST 0.41 ft03:44 PM EST 6.91 ft10:02 PM EST 0.02 ft06:39 AM EST05:30 PM EST02:46 PM EST01:57 AM EST
    Mon 0304:11 AM EST 7.13 ft10:30 AM EST 0.16 ft04:42 PM EST 7.00 ft10:56 PM EST −0.28 ft06:40 AM EST05:29 PM EST03:26 PM EST03:02 AM EST
    Tue 0405:09 AM EST 7.49 ft11:27 AM EST −0.07 ft05:36 PM EST 7.08 ft11:47 PM EST −0.51 ft06:41 AM EST05:28 PM EST04:06 PM EST04:07 AM EST
    Wed 0506:02 AM EST 7.78 ft12:21 PM EST −0.21 ft06:26 PM EST 7.10 ft06:42 AM EST05:28 PM EST04:48 PM EST05:12 AM EST
    Thu 0612:36 AM EST −0.62 ft06:51 AM EST 7.94 ft01:13 PM EST −0.25 ft07:14 PM EST 7.03 ftFull Moon06:43 AM EST05:27 PM EST05:32 PM EST06:15 AM EST
    Fri 0701:24 AM EST −0.61 ft07:38 AM EST 7.92 ft02:02 PM EST −0.18 ft08:00 PM EST 6.86 ft06:44 AM EST05:26 PM EST06:19 PM EST07:18 AM EST
    Sat 0802:10 AM EST −0.48 ft08:23 AM EST 7.74 ft02:48 PM EST −0.00 ft08:47 PM EST 6.61 ft06:44 AM EST05:25 PM EST07:08 PM EST08:18 AM EST
    Sun 0902:54 AM EST −0.22 ft09:09 AM EST 7.43 ft03:32 PM EST 0.27 ft09:34 PM EST 6.30 ft06:45 AM EST05:25 PM EST07:59 PM EST09:14 AM EST
    Mon 1003:38 AM EST 0.12 ft09:55 AM EST 7.06 ft04:14 PM EST 0.60 ft10:22 PM EST 5.99 ft06:46 AM EST05:24 PM EST08:52 PM EST10:05 AM EST
    Tue 1104:21 AM EST 0.51 ft10:41 AM EST 6.68 ft04:57 PM EST 0.94 ft11:12 PM EST 5.73 ft06:47 AM EST05:23 PM EST09:45 PM EST10:52 AM EST
    Wed 1205:05 AM EST 0.91 ft11:30 AM EST 6.35 ft05:42 PM EST 1.23 ft06:48 AM EST05:23 PM EST10:38 PM EST11:34 AM EST
    Thu 1312:04 AM EST 5.54 ft05:52 AM EST 1.25 ft12:19 PM EST 6.09 ft06:30 PM EST 1.44 ft06:49 AM EST05:22 PM EST11:31 PM EST12:12 PM EST
    Fri 1412:55 AM EST 5.47 ft06:46 AM EST 1.48 ft01:08 PM EST 5.92 ft07:22 PM EST 1.51 ftLast Quarter06:50 AM EST05:21 PM EST12:48 PM EST
    Sat 1501:46 AM EST 5.49 ft07:44 AM EST 1.56 ft01:57 PM EST 5.83 ft08:15 PM EST 1.44 ft06:51 AM EST05:21 PM EST12:24 AM EST01:22 PM EST
    Sun 1602:36 AM EST 5.62 ft08:42 AM EST 1.49 ft02:47 PM EST 5.80 ft09:05 PM EST 1.26 ft06:52 AM EST05:20 PM EST01:16 AM EST01:55 PM EST
    Mon 1703:28 AM EST 5.83 ft09:37 AM EST 1.30 ft03:38 PM EST 5.85 ft09:53 PM EST 1.01 ft06:52 AM EST05:20 PM EST02:09 AM EST02:27 PM EST
    Tue 1804:19 AM EST 6.11 ft10:29 AM EST 1.04 ft04:29 PM EST 5.95 ft10:40 PM EST 0.71 ft06:53 AM EST05:19 PM EST03:03 AM EST03:01 PM EST
    Wed 1905:08 AM EST 6.44 ft11:18 AM EST 0.75 ft05:18 PM EST 6.10 ft11:25 PM EST 0.42 ft06:54 AM EST05:19 PM EST03:59 AM EST03:37 PM EST
    Thu 2005:53 AM EST 6.77 ft12:06 PM EST 0.46 ft06:04 PM EST 6.25 ft06:55 AM EST05:19 PM EST04:56 AM EST04:15 PM EST
    Fri 2112:10 AM EST 0.15 ft06:37 AM EST 7.06 ft12:53 PM EST 0.20 ft06:48 PM EST 6.37 ft06:56 AM EST05:18 PM EST05:54 AM EST04:58 PM EST
    Sat 2212:56 AM EST −0.07 ft07:19 AM EST 7.26 ft01:40 PM EST 0.00 ft07:32 PM EST 6.43 ftNew Moon06:57 AM EST05:18 PM EST06:54 AM EST05:46 PM EST
    Sun 2301:42 AM EST −0.23 ft08:03 AM EST 7.36 ft02:27 PM EST −0.13 ft08:18 PM EST 6.42 ft06:58 AM EST05:17 PM EST07:53 AM EST06:39 PM EST
    Mon 2402:29 AM EST −0.32 ft08:49 AM EST 7.36 ft03:13 PM EST −0.18 ft09:06 PM EST 6.36 ft06:59 AM EST05:17 PM EST08:51 AM EST07:36 PM EST
    Tue 2503:16 AM EST −0.31 ft09:38 AM EST 7.26 ft04:01 PM EST −0.15 ft09:58 PM EST 6.28 ft07:00 AM EST05:17 PM EST09:46 AM EST08:38 PM EST
    Wed 2604:06 AM EST −0.20 ft10:32 AM EST 7.10 ft04:50 PM EST −0.06 ft10:55 PM EST 6.22 ft07:00 AM EST05:17 PM EST10:36 AM EST09:41 PM EST
    Thu 2704:58 AM EST −0.01 ft11:29 AM EST 6.92 ft05:44 PM EST 0.06 ft11:56 PM EST 6.23 ft07:01 AM EST05:16 PM EST11:23 AM EST10:46 PM EST
    Fri 2805:56 AM EST 0.21 ft12:29 PM EST 6.75 ft06:42 PM EST 0.13 ft07:02 AM EST05:16 PM EST12:06 PM EST11:50 PM EST
    Sat 2912:57 AM EST 6.32 ft07:01 AM EST 0.38 ft01:27 PM EST 6.60 ft07:42 PM EST 0.10 ftFirst Quarter07:03 AM EST05:16 PM EST12:47 PM EST
    Sun 3001:56 AM EST 6.48 ft08:09 AM EST 0.42 ft02:25 PM EST 6.48 ft08:42 PM EST −0.03 ft07:04 AM EST05:16 PM EST01:26 PM EST12:54 AM EST

    Thursday, November 6, 2014

    Resource Post

    This video helped me understand Newton's Third Law much better because the professor did several examples in everything he explained, and also asked questions as to why certain things happened. It allowed me to visualize each concept and see why things happened. For example, leaning on the table standing versus leaning on the table on a skateboard. He has each of his objects handy and didn't have to waste anytime to get them out. He was efficient in explaining and got a lot done in a short amount of time. At the same time, this isn't always the best route because often times students are confused and it'd be easier to slow down for those who didn't catch everything he says. Plus they wouldn't have to backtrack if someone was lost. This is a college course, but looking in as a high school student, this is a different way of teaching.

    Monday, October 27, 2014

    Unit 2

    A. Newton's Second Law
    • Can be defined as a=f/m
      • This is the same as a=f*/(1/m) 
    • Describes the relationship between acceleration and mass and the relationship between acceleration and force
      • Force is directly proportional to acceleration
        • This means that as force goes up acceleration goes up
      • Mass is indirectly proportional to acceleration
        • This means that as mass goes up acceleration goes down


    B. Newton's Second Law Lab
    • In the first lab we manipulated the mass of the system by adding mass to the cart an leaving the force/mass of the hanger the same
    • As mass increased, the acceleration went down
    • When we graphed the line of the data we gathered, we found the slope to be .468 
    • The force from the hanger was .5N 
    • The reason why they are so close is because the force was the constant so it will also be the slope of the line

    Friday, September 26, 2014

    Unit 1

    Inertia/Newton’s 1st Law
    • .An object at rest will stay at rest until a force is acted upon it
      • The friction between the paper and cup isn't enough to make the cup move though the paper was snatched from under it
        • Inertia is a property that states that an objects state of motion remains the same
    • An object in motion will stay in motion unless a force is acted upon it to stop it
    • An object with a lot of mass will also have a lot of inertia
    Net force and Equilibrium
    • Net Force is the total force being acted upon an object
      • Force is a push or pull
        • Force is measured in newtons, or N
      • When net force equals 0, the object is at an equilibrium
        • Equilibrium can occur at two different times
          • When the object is at rest, and when the object is moving at a constant velocity
          • When an object is at equilibrium, the forces canceled each other out
          • I push 5N to the left and you push 5N to the right,
      • Ex: I push 5N to the left and you push 10N to the right the net force on this object is 5N to the right
    Velocity
    • Speed and velocity are not the same thing
      • Speed is how fast something is going at a certain rate
      • Velocity is how fast something is going at a certain rate but it adds the magnitude direction
      • An object can go at a consistent speed and not have a constant velocity because velocity has direction
    • v=d/t
    • When velocity is changing, the object is accelerating
    • Arrows which are vectors can be used to show an objects direction and how big it is can show you how fast it is going
    • Ex= Ike is goes 6 meters after 2 seconds. How fast is he going?
      • 6m/2s= 3m/2

    Acceleration
    • .Acceleration= ⌂v/t
    • Acceleration is the rate at which something changed velocity
    • If something has a constant velocity,it cannot have an acceleration
    • If something is accelerating therefore, it cannot have a constant velocity
    • The units for acceleration are m/s^2
    • The rate of acceleration in free fall is equal to 9.8 m/s^2
      • This is gravity and it is constant
    • When you are driving on the highway and you start to speed up you are accelerating
    • When you are on cruise control you are not
    Using a graph
    • When given distance and time an object was in motion, we can find out the acceleration as well as the velocity
      • The y axis must have distance
      • The x axis must have time or time^2
        • If the time is 3 then time^2 equals 3*3=9
    • When acceleration is constant
      • The graph with time will be exponential 
      • The graph with time squared will be linear
        • This slope will be equal to the 1a/2 in d=(1a/2)t^2
    • When velocity is constant
      • The line will be linear
      • The slope is equal to the velocity
        • This is because v=d/t
    • When you use a scatter plot for your data, you must make a best fit line
      • It should be the median with all of your points and can give you a solid idea of where the line may be in later point
      • The slope of the best fit line also tells you the correlation of your plot based on its sign