forces and motion
DESCRIPTION
Forces and motion. Speed. metres. Speed = distance travelled time taken. Metres per second (m/s). seconds. Speed. kilometres. Speed = distance travelled time taken. Kilometres per hour (km/h). hours. d. s. t. x. triangle. No movement. distance. time. Constant speed. - PowerPoint PPT PresentationTRANSCRIPT
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Forces and motion
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Speed
Speed = distance travelledtime taken
seconds
metres
Metres per second (m/s)
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Speed
Speed = distance travelledtime taken
hours
kilometres
Kilometres per hour (km/h)
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triangle
s tx
d
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No movement
distance
time
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Constant speed
distance
time
fast
slow
The gradient of the graph gives the
speed
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Getting faster (accelerating)
distance
time
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A car accelerating from stop and then hitting a wall
distance
time
Let’s try a simulation
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Speed against time graphs
speed
time
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No movement
speed
time
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Constant speed
speed
time
fast
slow
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Getting faster? (accelerating)
speed
time
Constant acceleration
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Getting faster? (accelerating)
speed
time
a = v – u
t
(v= final speed, u = initial speed)
v
u
The gradient of this graph gives the acceleration
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Getting faster? (accelerating)
speed
time
The area under the graph gives the distance travelled
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A dog falling from a tall building (no air resistance)
speed
time
Area = height of building
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Forces
• Remember a force is a push (or pull)
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Forces
• Force is measured in Newtons
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Forces
• There are many types of forces; electrostatic, magnetic, upthrust, friction, gravitational………
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Which of the following is the odd one out?
MassSpeedForce
TemperatureDistanceElephant
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Scalars and vectors
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Scalars
Scalar quantities have a magnitude (size) only.
For example:
Temperature, mass, distance, speed, energy.
1 kg
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Vectors
Vector quantities have a magnitude (size) and direction.
For example:
Force, acceleration, displacement, velocity, momentum.
10 N
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Scalars and Vectors
scalarsvectors
Magnitude (size)
No direction
Magnitude and direction
temperature mass
speed
velocity
forceacceleration
Copy please!
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Representing vectors
Vectors can be represented by arrows. The length of the arrow indicates the magnitude, and the direction the direction!
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Adding vectors
When adding vectors (such as force or velocity) , it is important to remember they are vectors and their direction needs to be taken into account.
The result of adding two vectors is called the resultant.
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Adding vectors
For example;
6 N 4 N 2 N
Resultant force
Copy please!
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An interesting example
velocity
We have constant speed but changing velocity.
Of course a changing velocity means it must be accelerating! We’ll come back to this in year 12!
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Friction opposes motion!
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Newton’s 1st Law
If there is no resultant force acting on an object, it will move with constant velocity. (Note the constant velocity could be zero).
Does this make sense?
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Newton’s second law
Newton’s second law concerns examples where there is a resultant force.
I thought of this law myself!
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Newton’s 2nd law
There is a mathematical relationship between the resultant force and acceleration.
Resultant force (N) = mass (kg) x acceleration (m/s2)
FR = maIt’s physics,
there’s always a mathematical relationship!
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An example
Resultant force = 100 – 60 = 40 NFR = ma
40 = 100aa = 0.4 m/s2
Pushing force (100 N)
Friction (60 N)
Mass of Mr Porter and bike = 100 kg
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Newton’s 3rd lawIf a body A exerts a force on body B, body B will exert an equal but opposite force on body A.
Hand (body A) exerts force on table (body B)
Table (body B) exerts force on hand (body A)
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Gravity
Gravity is a force between ALL objects!
Gravity
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Gravity
Gravity is a very weak force.
The force of gravitational attraction between Mr Porter and his wife (when 1 metre apart) is only around 0.0000004 Newtons!
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Gravity
The size of the force depends on the mass of the objects. The bigger they are, the bigger the force!
Small attractive force
Bigger attractive force
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Gravity
The size of the force also depends on the distance between the objects.
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Gravity
The force of gravity on something is called its weight. Because it is a force it is measured in Newtons.
Weight
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Gravity
On the earth, Mr Porter’s weight is around 800 N.
800 N
I love physics!
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Gravity
On the moon, his weight is around 130 N.Why?
130 N
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Mass
Mass is a measure of the amount of material an object is made of. It is measured in kilograms.
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Mass
Mr Porter has a mass of around 77 kg. This means he is made of 77 kg of blood, bones, hair and poo!
77kg
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Mass
On the moon, Mr Porter hasn’t changed (he’s still Mr Porter!). That means he still is made of 77 kg of blood, bones, hair and poo!
77kg
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Mass and weight
Mass is a measure of the amount of material an object is made of. It is measured in kilograms.
Weight is the force of gravity on an object. It is measured in Newtons.
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Calculating weight
To calculate the weight of an object you multiply the object’s mass by the gravitational field strength wherever you are.
Weight (N) = mass (kg) x gravitational field strength (N/kg)
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Gravity = air resistanceTerminal velocity
gravity
As the dog falls faster and air resistance increases, eventually the air resistance becomes as big as (equal to) the force of gravity.
The dog stops getting faster (accelerating) and falls at constant velocity.
This velocity is called the terminal velocity.
Air resistance
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Falling without air resistance
gravity
Without air resistance objects fall faster and faster and faster…….
They get faster by 10 m/s every second (10 m/s2)
This number is called “g”, the acceleration due to gravity.
Can you copy the words please?
Where did I come from?
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Falling without air resistance?
distance
time
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Falling without air resistance?
speed
time
Gradient = acceleration = 9.8 m.s-2
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Falling with air resistance?
distance
time
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Falling with air resistance?
speed
time
Terminal speed
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Stopping distances
The distance a car takes to stop is called the stopping distance.
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Two parts
The stopping distance can be thought of in two parts
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Stopping distancesThinking distance is the distance traveled whilst the driver is thinking (related to the driver’s reaction time).
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Thinking distance
This is affected by the mental state of the driver (and the speed of the car)
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Braking distance
This is the distance traveled by the car once the brakes have been applied.
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Braking distance
This affected by the speed and mass of the car
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Braking distance
It is also affected by the road conditions
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Braking distance
And by the condition of the car’s tyres.
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Typical Stopping distances YouTube - Top Gear 13-5: RWD Braking Challenge
YouTube - Think! - Slow Down (Extended) (UK)
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Momentum
• What makes an object hard to stop? • Is it harder to stop a bullet, or a truck
travelling along the highway?
• Are they both as difficult to stop as each other?
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Momentum
• Momentum is a useful quantity to consider when thinking about "unstoppability". It is also useful when considering collisions and explosions. It is defined as
Momentum (kgm/s) = Mass (kg) x Velocity (m/s)
p = mv
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An easy example
• A lorry has a mass of 10 000 kg and a velocity of 3 m/s. What is its momentum?
Momentum = Mass x velocity = 10 000 x 3 = 30 000 kgm/s
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Law of conservation of momentum
• The law of conservation of linear momentum says that
“in an isolated system, momentum remains constant”.
We can use this to calculate what happens after a collision (and in fact during an “explosion”).
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Conservation of momentum
• In a collision between two objects, momentum is conserved (total momentum stays the same). i.e.
Total momentum before the collision = Total momentum after
Momentum is not energy!
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A harder example!
• A car of mass 1000 kg travelling at 5 m/s hits a stationary truck of mass 2000 kg. After the collision they stick together. What is their joint velocity after the collision?
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A harder example!
5 m/s
1000kg
2000kgBefore
AfterV m/s
Combined mass = 3000 kg
Momentum before = 1000x5 + 2000x0 = 5000 kgm/s
Momentum after = 3000v
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A harder exampleThe law of conservation of momentum tells us that
momentum before equals momentum after, so
Momentum before = momentum after5000 = 3000v
V = 5000/3000 = 1.67 m/s
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Momentum is a vector
• Momentum is a vector, so if velocities are in opposite directions we must take this into account in our calculations
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An even harder example!
Snoopy (mass 10kg) running at 4.5 m/s jumps onto a skateboard of mass 4 kg travelling in the opposite direction at 7 m/s. What is the velocity of Snoopy and skateboard after Snoopy has jumped on?
I love physics
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An even harder example!
10kg
4kg-4.5 m/s7 m/s
Because they are in opposite directions, we make one velocity negative
14kg
v m/s
Momentum before = 10 x -4.5 + 4 x 7 = -45 + 28 = -17
Momentum after = 14v
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An even harder example!
Momentum before = Momentum after-17 = 14v
V = -17/14 = -1.21 m/s
The negative sign tells us that the velocity is from left to right (we choose this as our “negative direction”)
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Impulse
Ft = mv – mu
The quantity Ft is called the impulse, and of course mv – mu is the change in momentum (v =
final velocity and u = initial velocity)
Impulse = Change in momentum
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Units
Impulse is measured in Ns
or kgm/s
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Impulse
Note; For a ball bouncing off a wall, don’t forget the initial and final velocity are in
different directions, so you will have to make one of them negative.
In this case mv – mu = 5m - -3m = 8m
5 m/s
-3 m/s
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Example• Jack punches Chris in the face. If Chris’s head (mass 10 kg) was
initially at rest and moves away from Jack’s fist at 3 m/s, and the fist was in contact with the face for 0.2 seconds, what was the force of the punch?
• m = 10kg, t = 0.2, u = 0, v = 3• Ft = mv – mu• 0.2F = 10x3 – 10x0• 0.2F = 30• F = 30/0.2 = 150N
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The turning effect of a force depends on two things;
The size of the force
Obviously!
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The turning effect of a force depends on two things;
The distance from the pivot (axis of rotation)
Not quite so
obvious!
Axis of rotation
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Turning effect of a force – moment of a force
Moment (Nm) = Force (N) x distance from pivot (m)
Note the unit is Nm, not N/m!
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A simple example!
nut
spanner (wrench)
50 N
0.15 m
Moment = Force x distance from pivot
Moment = 50 N x 0.15 m
Moment = 7.5 Nm
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If the see-saw balances, the turning effect anticlockwise must equal the
turning effect clockwise
pivot
1.2 m 2.2 m
110 N? N
Anticlockwise moment clockwise moment=
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Anticlockwise moment = clockwise moment? X 1.2 = 110 x 2.2
? X 1.2 = 242? = 242/1.2? = 201.7 N
pivot
1.2 m 2.2 m
110 N? N
Anticlockwise moment clockwise moment=
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Principal of Moments
Rotational equilibrium is when the sum of the anticlockwise moments equal the sum of the clockwise moments.
YouTube - Alan Partridge's Apache office
COPY PLEASE!
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Centre of gravity
The centre of gravity of an object is the point where the object’s weight seems to act.
I think he wants you
to copy this
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Complex shapes
How do you find the centre of
gravity of complex shapes?
Complex shape man
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Finding the centre of mass
i. Place a compass or needle through any part of the card.
ii. Make sure that the card “hangs loose”.iii. Hang a plumb line on the needle.iv. After it has stopped moving, carefully draw a
line where the plumb line is.v. Place the needle in any other part of the card.vi. Repeat steps ii to iv.vii. Where the two drawn lines cross is where the
centre of mass is.viii. Physics is the most interesting subject.
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Hooke’s law
Force (N)
Extension (cm)
Elastic limit
The extension of a spring is proportional to the force applied (until the elastic limit is reached)
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Steel, glass and wood!Force
Extention
Even though they don’t stretch much, they obey Hooke’s law for the first part of the graph
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RubberForce
Extension
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The Solar System
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Main points
• Know the names of the planets!• My very easy method just speeds up naming
planets• They orbit in ellipses with the sun at one foci• Inner planets small and rocky• Outer planets large and mainly gas• Asteroid belt between Mars and Jupiter
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• Giant dirty snow balls (ice and dust) (diameter 100m - 50 km?)
• Very elliptical orbits• Short period (T < 200 yrs) and long period
(could be thousands of years)• Oort cloud• Tail(s) always point away from the sun• Evaporate as they get closer to the sun
Comets
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Orbital motion
• Space objects• use the relationship between orbital
speed, orbital radius and time period• orbital speed = 2× π ×orbital radius/(time
period)• v = 2× π × r
T
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My address
11507 Meadow Lake DriveHoustonTexas 77077USAEarthSolar System
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My address11507 Meadow Lake DriveHoustonTexas 77077USAEarthSolar SystemMilky wayLocal groupUniverse
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Galaxies
• A large collection of stars held together by their mutual gravity.
• Dwarf galaxies might have only a few million stars, many galaxies have hundreds of billions.
• The Universe has around 100 billion galaxies
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Orbital speed
• Speed = distance/time
• v = (2πr)/T
• r = radius of orbit• T = Period (time for one orbit)