Transcript SPIN

SPIN
Slides created by Kathy Buckland
at the University of British
What’s Happening Here?
• An example of circular motion
What is Circular Motion?
• The circular path along which an
object travels
• The rotation around a fixed axis
What is the word used to describe this
path?
ORBIT
Examples
•
•
•
•
Rollercoaster
Swinging an object on a string
Planetary objects-moon, satellites, etc.
Car going around a round-about
Back to the mid 1600’s…
Newton’s Second Law:
“Mutationem motus proportionalem esse vi motrici
impressae, et fieri secundum lineam rectam qua vis illa
imprimitur”
-Principia Mathematica (1687)
Otherwise known as…
F  ma
F=force (N)
m=mass (kg)
a=acceleration (m/s2)
F=ma
What is FORCE?
• PUSH
or a…
• PULL
Examples of Forces
• Gravity
• Impact Forces
• Tension
• Friction
Circular Motion and
Force
How does the object stay in its path?
This force is called…
CENTRIPETAL FORCE
centrum "center" and petere “go to” or
“seek”
To get where you want “to go”,
you must….
PEDAL….
Not a new force !!
Examples of forces:
• Gravity
• Impact Forces
• Tension
• Friction
Examples of these “acting” as the
CENTRIPETAL FORCE
• Ball on a string
• Rollercoaster
• Planetary Motion
• Car going in circles
F  ma
What next?
MASS
• The amount of MATTER an object contains
• Not weight -weight changes depending on
gravitation field
F  ma
and finally…
ACCELERATION
How the velocity changes in a certain
amount of time
In physics lingo
v
a
t
a=acceleration (m/s2)
Δ= “change in”
v=velocity (m/s)
t=time (s)
2007 Lamborghini
Murcielago LP640
acceleration: 0-62 mph time of 3.4 seconds
(0-100km/h in 3.4 seconds!)
F  ma
ACCELERATION
How the velocity changes in a certain amount of time
In physics lingo
•
•
•
•
a=acceleration (m/s2)
Δ= “change in”
v=velocity (m/s)
t=time (s)
v
a
t
• Velocity has a DIRECTION and a
MAGNITUDE
• The speed is the MAGNITUDE
How do we represent direction and
magnitude?
VECTORS
Vector Recall
The length of the vector represents the
MAGNITUDE or SPEED
The direction it points is the
DIRECTION
Adding:
a
a+b
b
Subtracting:
a
a-b
b
Back to Circular Motion…
F  ma
How can we find the force it takes to hold on
object in orbit?
Remember:
v
a
t
Δv is a change in direction not magnitude
DEMO # 1
Finding centripetal acceleration
What will it be?
How do we get centripetal
acceleration ?
A little geometry and algebra…
Find
similar triangles
t2
Three more steps..
1. Make a tiny triangle
so..
•
•
t1
S=v(t2-t1)=vΔt
have a right triangle
use sinθ = opposite
hypotenuse
•
sin θ = θ
2. Use similar triangles
3. Use some algebra
Centripetal acceleration
is…
2
v
acent 
r
Finally put it all together…
v
F  ma  m
t
For circular motion…
Fcent  macent
2
v
m
r
Now What’s Happening
Here?
• Our starting example of circular
motion
What to remember
• What circular motion is- be able to recognize it
• Newton’s Second Law- you will see it again!
F  ma
• That velocity has direction and speed
• Centripetal acceleration deals with the change in
direction
• Things that effect centripetal force are mass,
velocity, and the distance from the center
2
Fcent
v
m
r