Transcript Chapter 4: Forces and Newton`s Laws of Motion

Chapter 4
Forces and Newton’s Laws of Motion
MFMcGraw
PHY 1401- Ch 04 - Revised: 2/3/2010
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Forces and Newton’s Laws of
Motion
• Forces
• Newton’s Three Laws of Motion
• The Gravitational Force
• Contact Forces (normal, friction, tension)
• Application of Newton’s Second Law
• Apparent Weight
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Net Force
The net force is the vector sum of all the forces acting
on a body.
Fnet  F  F1  F2  F3  
The net force is the resultant of this vector addition.
Bold letters represent vectors. The units of Force are Newtons, or
the abbreviation N, which represent the SI units: kg-m/s2
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Free Body Diagrams
The free body diagram (FBD) is a simplified representation of an object, and the
forces acting on it. It is called free because the diagram will show the object without
its surroundings; i.e. the body is “free” of its environment.
We will consider only the forces acting on our object of interest. The object is
depicted as not connected to any other object – it is “free”. Label the forces
appropriately. Do not include the forces that this body exerts on any other body.
The best way to explain the free body diagram is to describe the steps required to
construct one. Follow the procedure given below.
(1) Isolate the body of interest. Draw a dotted circle around the object that
separates our object from its surroundings.
(2) Draw all external force vectors acting on that body.
(3) You may indicate the body’s assumed direction of motion. This does not
represent a separate force acting on the body.
(4) Choose a convenient coordinate system.
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Free Body Diagram
y
N1
The force directions are as
indicated in the diagram.
The magnitudes should be
in proportion if possible.
F
T
x
w1
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Newton’s First Law of Motion:
Inertia and Equilibrium
Newton’s 1st Law (The Law of Inertia):
If no force acts on an object, then the speed and
direction of itsmotion do not change.
Inertia is a measure of an object’s resistance to
changes in its motion.
It is represented by the inertial mass.
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Newton’s First Law of Motion
If the object is at rest, it remains at rest (velocity = 0).
If the object is in motion, it continues to move in a
straight line with the same velocity.
No force is required to keep a body in straight line
motion when effects such as friction are negligible.
An object is in translational equilibrium if the net
force on it is zero and vice versa.
Translational Equilibrium
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Newton’s Second Law of Motion
Net Force, Mass, and Acceleration
Newton’s 2nd Law:
The acceleration of a body is directly proportional to
the net force acting on the body and inversely
proportional to the body’s mass.
Mathematically:
Fnet
a
or Fnet  ma
m
This is the workhorse of mechanics
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Newton’s Second Law of Motion
An object’s mass is a measure of its inertia. The
more mass, the more force is required to obtain a
given acceleration.
The net force is just the vector sum of all of the
forces acting on the body, often written as F.
If a = 0, then F = 0. This body can have:
Velocity = 0 which is called static equilibrium, or
Velocity  0, but constant, which is called dynamic
equilibrium.
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Newton’s Third Law of Motion
Interaction Pairs
Newton’s 3rd Law:
When 2 bodies interact, the forces on the bodies,
due to each other, are always equal in magnitude
and opposite in direction.
In other words, forces come in pairs.
Mathematically:
F21  F12.
designates the force on object 2 due to object 1.
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Types of Forces
Contact forces: Normal Force & Friction
Tension
Gravitational Force
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Contact Forces
Contact forces: these are forces that arise due
to of an interaction between the atoms in the
surfaces of the bodies in contact.
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Normal Forces
Normal force: this force acts in the direction perpendicular
to the contact surface.
N
Normal force of the
ground on the box
N
w
Normal force
of the ramp
on the box
w
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Normal Forces
y
N
Example: Consider a
box on a table.
FBD for
box
x
w
Apply
Newton’s
2nd law
F
y
 N w0
So that N  w  mg
This just says the magnitude of the normal force
equals the magnitude of the weight; they are not
Newton’s third law interaction partners.
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Frictional Forces
Friction: a contact force parallel to the contact surfaces.
Static friction acts to prevent objects from sliding.
Kinetic friction acts to make sliding objects slow
down. Sometimes called Dynamic friction.
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Frictional Forces
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Tension
This is the force transmitted through a “rope”
from one end to the other.
An ideal cord has zero mass, does not stretch,
and the tension is the same throughout the cord.
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Example (text problem 4.77): A pulley is hung from the ceiling by a rope.
A block of mass M is suspended by another rope that passes over the
pulley and is attached to the wall. The rope fastened to the wall makes a
right angle with the wall. Neglect the masses of the rope and the pulley.
Find the tension in the rope from which the pulley hangs and the angle .
y
T
FBD for the
mass M
x
w
Apply Newton’s 2nd
Law to the mass M.
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F
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y
T w0
T  w  Mg
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Example continued:
Apply Newton’s 2nd Law:
FBD for the pulley:
F
F
y
y
 F sin   T  0

x
T
MFMcGraw
 F cos   T  0
T  F cos  F sin 
F
T
x
This statement is true
only when  = 45 and
F  2 T  2 Mg
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Gravitational Forces
Gravity is the force between two masses. Gravity is a
long-range force. No contact is needed between the
bodies. The force of gravity is always attractive!
GM1M 2
F
r2
M1
r is the distance between the two masses
M1 and M2 and G = 6.671011 Nm2/kg2.
F21
F12
M2
F21  F12.
r
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Gravitational Forces
 GM E
F  2
 r
Let M1 = ME = mass of the Earth.

M 2

Here F = the force the Earth exerts on mass M2. This is the
force known as weight, w.
 GM E
w   2
 rE

 M 2  gM 2 .

M E  5.98 10 24 kg
rE  6400 km
GM E
where g  2  9.8 N/kg  9.8 m/s 2
rE
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Near the surface of
the Earth
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Gravitational Forces
F
Note that g 
m
is the gravitational force per unit mass. This is called
the gravitational field strength. It is also referred to as
the acceleration due to gravity.
What is the direction of g?
What is the direction of w?
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Gravitational Forces
Example: What is the weight of a 100 kg astronaut on the
surface of the Earth (force of the Earth on the astronaut)?
How about in low Earth orbit? This is an orbit about 300
km above the surface of the Earth.
On Earth:
w  mg  980 N
 GM E 
  890 N
In low Earth orbit: w  mg (ro )  m
2 
 RE  h  
The weight is reduced by about 10%.
The astronaut is NOT weightless!
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Applying Newton’s Second Law
The one equation everyone remembers!
F  ma
Sumof the forces
acting on the objects
in the system
“m” is the
System
Mass
“a” is the
System
Response
This equation is just the tip of the “iceberg” of the mechanics
problem. The student will need to anlyze the forces in the
problem and sum the force vector components to build the
left hand side of the equation.
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Applying Newton’s Second Law
Example: A force of 10.0 N is applied to the right on block 1.
Assume a frictionless surface. The masses are m1 = 3.00 kg
and m2 = 1.00 kg.
Find the tension in the cord connecting the two blocks as
shown.
block 2
block 1
F
Assume that the rope stays taut so that both blocks
have the same acceleration.
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FBD for block 2:
FBD for block 1:
y
y
N1
N2
F
T
T
x
x
w1
w2
Apply Newton’s 2nd Law to each block:
F
F
MFMcGraw
x
 T  m2 a
y
 N 2  w2  0
F
F
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x
 F  T  m1a
y
 N1  w1  0
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Example continued:
F  T  m1a (1)
These two equations contain
the unknowns: a and T.
T  m2 a (2)
To solve for T, a must be eliminated. Solve for a in (2)
and substitute in (1).
T 
F  T  m1a  m1  
 m2 
T 
 m1 
T
F  m1    T  1 
 m2 
 m2 
T
MFMcGraw
F
10 N

 2.5 N
 m1   3 kg 
1 
 1 

 m2   1 kg 
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Pick Your System Carefully
y
y
N1
N2
T
F
T
x
x
w2
w1
Include both objects in the system. Now when you sum
the x-components of the forces the tensions cancel. In
addition, since there is no friction, y-components do not
contribute to the motion.
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Apparent Weight
Stand on a bathroom scale.
y
FBD for the
person:
N
Apply Newton’s 2nd Law:
x
w
MFMcGraw
F
y
 N  w  ma y
N  mg  ma y
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Apparent Weight
The normal force is the force the scale exerts on you. By
Newton’s 3rd Law this is also the force (magnitude only)
you exert on the scale. A scale will read the normal force.
N  mg  a y 
is what the scale reads.
When ay = 0, N = mg. The scale reads your true weight.
When ay  0, N > mg or N < mg.
In free fall ay = -g and N = 0. The person is weightless.
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Apparent Weight
Example (text problem 4.128):
A woman of mass 51 kg is standing in an elevator. The elevator
pushes up on her feet with 408 newtons of force.
What is the acceleration of the elevator?
FBD for
woman:
y
Apply Newton’s 2nd Law: (1)
N
x
w
MFMcGraw
F
y
 N  w  ma y
N  mg  ma y
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Apparent Weight
Example continued:
Given: N = 408 newtons, m = 51 kg, g = 9.8 m/s2
Unknown: ay
Solving (1) for ay:
N  mg
ay 
 1.8 m/s 2
m
The elevator could be (1) traveling upward with decreasing
speed, or (2) traveling downward with increasing speed.
The change in velocity is DOWNWARD.
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Force Summary
Friction
Tension
Opposes motion
No mass
Proportional to normal
force
No stretching
Non-conservative
Pulleys
Massless
Static & dynamic
No friction (bearing)
Normal Forces
Perpendicular to surface
at point of contact.
Tension in rope
continuously changes
direction
Magnitude needed to
maintain equilibrium
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Summary
•
Newton’s Three Laws of Motion
•
Drawing free body diagrams
•
Contact forces versus long-range forces
•
Different forces (gravity, friction, normal, tension,
air resistance)
•
Application of Newton’s Second Law
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