∆ r
∆ t
=
Momentum
( f
− v i
∆ t
)
= r net alternative statement of
Newton’s second law
The time rate of change of momentum of an object is equal to the net force acting on it p t
I r
When a single, constant force F acts on the object for time ∆ t, there is an impulse
I r delivered to the object:
= r
F
∆ t = area under F-t curve
F
I r
Using
= r
F
∆ r
=
∆ r
=
∆ t m ( v r f
− v r i
)
=
Impulse r
F
∆ t t
Momentum is conserved for the system of objects. You must define the isolated system
Assumes only internal forces are acting during the collision
Can be generalized to any number of objects
Momentum is conserved in any collision
Inelastic collisions
Kinetic energy is not conserved
Some of the kinetic energy is converted into other types of energy such as heat, sound, work to permanently deform an object
Perfectly inelastic collisions occur when the objects stick together
Not all of the KE is necessarily lost
• The average angular speed, ω , of a rotating rigid object is the ratio of the angular displacement to the time interval
av
f
t f
t i i
t
Unit: rad/s
object is defined as the ratio of the change in the angular speed to the time it takes for the object to undergo the change:
av
f
t f
t i i
t
Unit: rad/s 2
• Displacements
s
r
• Speeds v t
r
• Every point on the rotating object has the same angular motion
• Not every point on the rotating object has the same linear motion
• Accelerations a t
r
T
2
2 v r f
1
T
2
Time to go around once v
Centripetal Acceleration
– The magnitude of the centripetal acceleration is given by a c
v t
2 r
– This direction is toward the center of the circle
The angular velocity and the linear velocity are related ( v t
= ω r )
The centripetal acceleration can also be related to the angular velocity a c
2 r
• General equation F c
m a c
m v
2 r
• If the force vanishes, the object will move in a straight line tangent to the circle of motion
of the acceleration is due to changing speed a t
a c
a
a t a to changing direction c
• Total acceleration can be found from these components a
a t
2 a
2
C
Don’t confuse: a t
r a c v
2
r
2 r
Newton’s Law of Universal Gravitation
• Every particle in Universe attracts every other particle with force: directly proportional to product of masses inversely proportional to square of distance between them.
F
G m
1 m
2
2 r inverse square law
G
= universal gravitational constant
= 6.673 x 10 -11 N m² /kg²
Applications of Universal Gravitation
Gravitational force of uniform sphere on particle outside sphere same as force exerted if entire mass of the sphere concentrated at its center--Gauss’ Law
• Acceleration due to gravity
• g will vary with altitude g
G
M r
2
E
Gravitational Potential Energy
• PE = mgy is valid only near the earth’s surface
• For objects high above the earth’s surface, an alternate expression is needed
PE
G
M
E m r
– Zero reference level is infinitely far from the earth
Escape Speed
• speed needed for an object to “escape” from planet
• For the earth, v esc
11.2 km/s is about
• Note, v is independent of the mass of the object v esc
2 GM
E
R
E
Ch. 8 General Torque Formula
Component of F
r
OR r F sin
• The lever arm , d , is the perpendicular distance from the axis of rotation to a line drawn along the direction of the force d = r sin
so
= F d = F r sin
Torque and Equilibrium
• First Condition of Equilibrium
F x
0
or
0 and
F y
0
•The Second Condition of Equilibrium states
0
• If an object is “symmetrical’’ then the center of mass is just where you think that it should be.
• If an object is “complicated” then
r
m
M
R
CoM
The torque from gravity is “as if” the force of gravity acts only at the CoM
Torque and Angular Acceleration
Newton’s Second Law for a Rotating Object
I analogous to
F = ma
I = moment of inertia
For Uniform Ring
I m r 2 MR 2 moment of inertia depends on quantity of matter and its distribution and location of axis of rotation
Other Moments of Inertia