Chapters Two and Three
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Transcript Chapters Two and Three
Chapter Two and
Chapter Three
Objectives
What is Motion?
Measuring Motion
Artstotle’s views
Horizontal versus Vertical Motion
Newton’s Laws of Motion
Momentum
Circular Motion
Law of Gravition
Motion and Measuring Motion
Change in position
Passage of time
Measuring Motion
Speed
Distance/time
Instantaneous versus Average
Velocity
Acceleration
Change of velocity/ time
Acceleration versus Deacceleration
Motion Examples
Speed: Example 2.1
Acceleration: Example 2.3
Aristotle’s Views
Two spheres
Sphere of perfection versus Sphere of change
Natural versus Forced Motion
Elements: earth, air, fire, and water
Reqired force by people
Could not explain interaction at a distance
Horizontal versus Vertical
Motion
Horizontal
Leaning Tower of Pisa
Rolling Balls
Inertia
Vertical
Free fall
Galileo versus Aristotle
Constant versus Accelerating objects
Horizontal versus Vertical
(cont.)
Vertical (cont.)
D=(1/2)at2
Confirmed with rolling ball
A=g=9.8 m/s2
T=(2d/g)
Compound Motion
A combination of vertical and horizontal motion
Newton’s Laws of Motion
Edmund Halley
Christmas Day, 1642
Trinity College, Cambridge
Halley: Principia, planetary motion
Well accepted
Newton’s First Law of Motion
“Every object retains it state of motion of its
stat of uniform straight-line motion unless
acted up by an unbalanced force”
Inertia
Mass
Newton’s Second Law of
Motion
“The acceleration of an object is directly
proportional to the net force acting on it and
inversely proportional to the mass of the
object”
Weight is a force
F = ma
Newton’s Third Law of Motion
“Whenever two objects interact, the force
exerted on one object is equal in size and
opposite in direction to the force exerted on
the other object”
Example: Standing on the Floor
FAB = FBA
Newton Examples
Second Law: Example 3.1
Third Law: Example 3.5
Momentum
“The total momentum of a group of
interacting objects remains the same in the
absence of external forces”
P=mv
Unusual
P gives no clues
Kg m/s has no other name
Circular Motion
Centripetal versus Centrifugal
No true Centrifugal
All circular motion inside
ac=v2/r
F=mv2/r
Newton’s Laws of Gravitation
“Every object in the universe is attractedto
every other object with a force that is directly
proportional to the product of their masses”
F = GM1M2/R2
G = 6.67 X 10-11 Nm2/kg2
Force and Gravitation Examples
Circular Motion: Example 3.7
Gaviation: Example 3.9, 3.10
Homework
Chapter Two
Questions for Thought
1, 6, 9
Parallel Exercise
3, 5
Chapter Three
Questions for Thought
1, 4, 9
Parallel Exercise
4, 10