r ( ) −

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∆ 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

Impulse

„

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

Collision of 2 objects

Conservation of Momentum

„

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

Types of Collisions

„

„

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

Average Angular Speed

• 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

Average Angular Acceleration

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

Relationship Between Angular and

Linear Quantities

• 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

Analogies Between Linear and

Rotational Motion

Period and Frequency

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

Nonuniform circular 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

Center of mass and of gravity

• 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

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