Rotational Motion

April 14, 2019 | Author: Gutsy | Category: Rotation Around A Fixed Axis, Torque, Angle, Force, Mechanical Engineering
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Stuff on rotational motion...

Description

 

R-1

Rotational Motion We are going to consider the motion of a rigid body about a fixed axis of rotation.

(rads) 

The angle of rotation is measured in radians:

s r



(dimensionless)

 Notice that for a given angle , the ratio s/r is independent of the size of the circle.

s



s



r

o

Example: How many radians in 180 ? Circumference C = 2  r  r  s o rad = 57.3    =   rads  rads = 180o, 1 rad r r 

s =  r



r

Angle  of a rigid object is measured relative to some reference orientation, just like 1D position x is measured relative to some reference position (the origin). Angle  is the "rotational position". Like position x in 1D, rotational  position  has a sign convention. Positive angles are CCW (counterclockwise).

Definition of angular velocity: velocity:   units    =

x



x+ x



0

d dt

,

=



 (rad/s) t

( like v 

dx dt

, v 

x ) t

rad s

In 1D, velocity v has a sign (+ or –  or – ) depending on direction. Likewise, for for fixed-axis rotation, rotation,  has a sign, depending on the sense of rotation. 

v: (+) ( –   – )

(+)

( –   – )

More generally, when the axis is not fixed, we define the vector angular velocity   with direction = the direction of the axis + "right hand rule". Curl fingers of right hand around rotation, thumb points in direction of vector.

11/8/2013

©University of Colorado at Boulder

 

R-2

For rotational motion, there is a relation between tangential velocity v (velocity along the rim) and angular velocity . s     s = r  , s in r r  time t  r  s v = r   v  = = r    t t

Definition of angular acceleration :     ( like a 

dv dt

a 

,

v ) t

Units:

d dt

 

,

    =

 (rad/s2 ) t

rad s2



= rate at which  is changing.  = constant   = 0  speed v along rim = constant = r  Equations for constant :

Recall from Chapter 2: We defined v =

and then showed that, if a = constant,

 Now, in Chapter 10, we define  =

So, if  = constant,

d dt

dx dt

dv

, a=

dt

 ,

v = v0  a t  2 x  x 0  v0 t  12 a t  2 2 v  v0  2 a (x  x 0 ) , =

d dt

.

 = 0   t  2 1   0  0 t  2  t  2 2   0  2  (  0 )

Same equations, just different symbols. Example: Fast spinning wheel with 0 = 50 rad/s ( 0 = 2f  f  8 rev/s ). Apply brake and wheel slows at  = 10 rad/s. How many revolutions before the wheel stops? 502 02 2 2 2 Use   0  2   , final = 0  0  0  2         125 rad 2 2(10)

125 rad 

1 rev 2 rad

11/8/2013

 19.9 rev

©University of Colorado at Boulder

 

R-3

Definition of tangential acceleration atan = rate at which speed v along rim is changing d(r ) dv d  atan = r  a tan  =  r  dt dt dt

atan is different than the radial or centripetal acceleration a r 

v

2





ar  is due to change in direction of velocity v atan is due to change in magnitude of velocity, speed v atan and ar  are the tangential and radial components of the acceleration vector a. a

atan

ar 

|a|  a 

a tan 2  a r 2

 

Angular velocity  also sometimes called angular frequency. Difference between angular velocity  and frequency f:

 

# radians sec

f  

,

# revolutions sec

T = period = time for one complete revolution (or cycle or rev)

 

2 rad T



2 T

,

f  

1 rev T



1 T





  2  f  -1

Units of frequency f = rev/s = hertz (Hz) . Units of angular velocity = rad /s = s

Example:  An old vinyl record disk with radius r = 6 in = 15.2 cm is spinning at 33.3 rpm

(revolutions per minute).  What

is the period T?

33.3 rev 1min



 

33.3 rev 60 s



60 s 33.3 rev

1rev

 1.80 s/rev

f = 1 / T = 1 rev / (1.80 s) = 0.555 Hz

is the angular velocity

11/8/2013

(60 / 33.3)s

period T = 1.80 s

What is the frequency f ?

 What



 ?

  2  f  2  (0.555 s 1)  3.49 rad / s

©University of Colorado at Boulder

   What

R-4 is the speed v of a bug hanging on to the rim of the disk? v = r

 =

-1

(15.2 cm)(3.49 s ) = 53.0 cm/s

 What

is the angular acceleration  of the bug?

 =

0 , since  = constant

 What

is the magnitude of the acceleration of the bug? The acceleration has only a radial

component ar  , since the tangential acceleration atan = r   = 0. a = a r  

v2 r



(0.530 m/s)2

 1.84 m/s2 (about 0.2 g's)

0.152 m

For every quantity in linear (1D translational) motion, there is corresponding quantity in rotational motion: Translation

x v

dx

a

dv



Rotation







 =

dt 

dt

 =

d dt d dt

F

 

(?)

M

 

(?)

F = Ma



(?) = (?) 



KE = (1/2) (?) 

KE = (1/2) m v

2

2

The rotational analogue of force is torque. Force F causes acceleration a

F = F sin



Torque  causes angular acceleration 



The torque (pronounced "tork") is a kind of

F axis

r

  r  F  r Fsin 

   r F  m N r = "lever arm" = distance from axis to point of application of force F = component of force perpendicular to lever arm

11/8/2013



F||

"rotational force". magnitude of torque:

F

©University of Colorado at Boulder

 

R-5

Example: Wheel on a fixed axis:  Notice that only the perpendicular component of the force F will rotate the wheel. The component of the force parallel to the lever arm (F||) has no effect on the rotation of the wheel. If you want to easily rotate an object about an axis, you want a large lever arm r and a large  perpendicular force F:

 best

 better

 bad axis

no good! (F = 0)

no good! r=0

Example: Pull on a door handle a distance r = 0.8 m from the hinge with a force of magnitude F o = 20 N at an angle  = 30  from the plane of the door, like so: F hinge

 =

F 

r F = r F sin  = o

(0.8 m)(20 N)(sin 30 ) = 8.0 m N

r  Another example: a Pulley

r



= r F

F

For fixed axis, torque has a sign (+ or – ) : Positive torque causes counter-clockwise CCW rotation.  Negative torque causes clockwise (CW) rotation.

+

 – 

If several torques are applied, the net torque causes angular acceleration: net 



 

Aside: Torque, like force, is a vector quantity. Torque has a direction. Definition of vector tor que   :   r  F = cross product of r and F: "r cross F" Vector Math interlude: The cross-product  of two vectors is a third vector A  B  C  defined like this: The magnitude of A  B is A B sin . The direction of A  B is the direction  perpendicular to the plane defined by the vectors A and B plus right-hand-rule. (Curl fingers from first vector A to second vector B, thumb points in direction of A  B

11/8/2013

©University of Colorado at Boulder

 

R-6

AB A



B

To see the relation between torque  and angular acceleration  , consider a mass m at the end of light rod of length r , pivoting on an axis like so:

m

r

axis

Apply a force F to the mass, keeping the force perpendicular to the lever arm r. F acceleration atan = r  F

axis

Apply Fnet = m a, along the tangential direction: F = m atan  = m r   2

Multiply both sides by r ( to get torque in the game ): r F  = (m r  )   2

Define "moment of inertia" = I = m r  



= I

( like F = m  a )

Can generalize definition of I: Definition of moment of inertia of an extended object about an axis of rotation:

I 



axis

mi ri 2  m1 r12  m2 r2 2   ...

r i m i

i

Examples:  2 small masses on rods of length r:

r

r m 11/8/2013

axis

2

I = 2 m r  m

©University of Colorado at Boulder

 

R-7

 A

2

hoop of total mass M, radius R, with axis through the center, has Ihoop = M R 

I 

m r

2

i i

i

 (m1  m2  m3 

mi

(since   r i = R for all i )

I  m1r12  m2 r2 2  m3r3 2 

In detail:



     mi  R 2  M R 2  i 

 m1R 2  m2 R 2  m3 R 2  

)R 2  MR 2

R

 

mass M

A solid disk of mass M, radius R, with axis through the center: 2

Idisk  = (1/2) MR  (need to do integral to prove this) R

See Appendix for I’s of various shapes. Moment of inertia I is "rotational mass". Big I

hard to get rotating



( like Big M

hard to get moving )



If I is big, need a big torque  to produce angular acceleration according to  net

= I

( like Fnet = m a )

Example: Apply a force F to a pulley consisting of solid disk of radius R, mass M.

 =

?

  I

R

RF 

F



1 2



MR 2   



 

2F M R 

Parallel Axis Theorem

Relates Icm (axis through center-of-mass) to I w.r.t. some other axis:

2

I = Icm + M d

(See proof in appendix.) Example: Rod of length L, mass M 1 ICM  M R 2 , d = L/2  12

Iend axis  ICM  M d  2

11/8/2013

1 12

ML  2

d

1 4

2

ML



1 3

2

ML

axis here (I)

rod mass M length L axis here ( Icm )

©University of Colorado at Boulder

 

R-8

Rotational Kinetic Energy How much KE in a rotating object? Answer: KErot  Proof:

KE tot 

(

1 2

1 2

I 2

( like KE trans 

1 2

m v2 )

mi vi 2 )

i

v  r ,

vi   ri



( 12 mi  ri 2 ) 

KE 

  1 2

i

axis

 2  2   mi ri     i 

1 2

r i m i

I 2

How much KE in a  rolling   wheel?

The formula v = r  is true for a wheel spinning about a fixed axis, where v is speed of points on rim. A similar formulas vCM



v

= r  works for a wheel rolling on the ground. Two very different situations, different v’s: v = speed of rim vs. vcm = speed of axis. But v = r  true for both.

v





v axis stationary: v =  r

vcm = center-of-mass velocity =  r

 point touching ground instantaneously at rest

To see why same formula works for both, look at situation from the bicyclist's point of view:

v



axis stationary, ground moving

v

11/8/2013

©University of Colorado at Boulder

 

R-9

Rolling KE: Rolling wheel is simultaneously translating and rotating: KEtot KE tot 

1 2

M v2 

1 2

+

=

I 2

=

KEtrans

+

KErot

(v = Vcm )

(See proof in appendix.)

Conservation of energy problem with rolling motion:

A sphere, a hoop, and a cylinder, each with mass M and radius R, all start from rest at the top of an inclined plane and roll down to the bottom. Which object reaches the bottom first? M

R (vi = 0)

h

vf  = v =? 

Apply Conservation of Energy to determine vfinal. Largest vfinal will be the winner.

 PEi

KEi



 Mgh 

0



KEf 1 2

Mv

2



1 2

PEf

 

I  0 2

KErot

KEtrans

Value of moment of inertia I depends on the shape of the rolling thing: 2

2

2

Idisk  = (1/2)M R   , Ihoop  = M R   , Isphere = (2 /5)M R  (Computing coefficient requires integral.) 2

Let's consider a disk, with I = (1/2)MR  . For the disk, the rotational KE is 2

1 2

I  2

1 2

v ( M R )    R 

 Mgh  gh 

3 4

2

1 2

1 2

v2 ,

M v2 

1 4

v 

1 4

M v2

[used   v / r]

M v 2  ( 12  14 )M v 2  4 3

g h  1.16

3 4

M v2

gh

 Notice that final speed does not depend on M or R.

11/8/2013

©University of Colorado at Boulder

 

R-10

Let's compare to final speed of a mass M, sliding down the ramp (no rolling, no friction). M

Mgh 

1 2

v =

2 g h  1.4 g h

M v2

(M's cancel)

(vi = 0) vf  = v =?

h 

Sliding mass goes faster than rolling disk. Why?

As the mass descends, PE is converted into KE. With a rolling object, KEtot = KEtrans + KErot , so some of the PE is converted into KE rot and less energy is left over for KEtrans. A smaller KEtrans 2

means slower speed (since KEtrans = (1/2) M v  ). So rolling object goes slower than sliding object, because with rolling object some of the energy gets "tied up" in rotation, and less is available for translation. Comparing rolling objects: Ihoop > Idisk  > Isphere



2

Hoop has biggest KErot = (1/2) I  , 

hoop ends up with smallest KEtrans  hoop rolls down slowest, sphere rolls down fastest.

Another conservation of rotational energy problem:

Rod of mass M, length L, one end stationary on ground, starts from rest at a ngle  and falls. What is speed v of end of stick, when stick hits ground?

I

L

1 3

M L2

(axis at end)

Plan: Use conservation of energy to get ,

CM hCM v=?



fixed axis

then v =  r =  L

Ei  E f



M g h CM 

1 2

I 2

Important point: PEgrav = Mgh where h = height of center-of-mass, independent of the orientation of the stick. Proof: PEgrav



m gh i

i

11/8/2013

i

 g mi h i  g M YCM  M g h CM i

©University of Colorado at Boulder

 

R-11

( Have used definition of center-of-

  mi yi )

mass: MYCM

same hCM , same PE

rav

i

Back to the problem: M g h CM

Mg Use

1 2

L sin  



M L2 2

1 1 2 3

1 2



I 2 ,

h  12 Lsin  , I 

g sin  

  v / r  v / L to get: 3g sin   L

v2 2

L

1 3

1 3

M L2

h 

L 2



L/2

v2 L



v

3g Lsin   Done.

The tip of the stick starts at height h tip = L sin, but its final speed v is faster than the speed of an object that falls from that height h [ 1 2

m v2  m g h



v

2g h ]. The tip of the stick falls faster

than it would in free-fall, because the central part of the rod pulls it down. This is why tall chimneys always break apart when toppled: : Let's Review:  Translation x v

dx

a

dv





 =



dt

M F = Ma KE = (1/2) m v

2

Rotation



dt

F

11/8/2013



  =







I







d dt d dt

=I 2

KE = (1/2) I 

©University of Colorado at Boulder

 

R-12

Appendix 1: Moments of Inertia for some shapes

R Hoop

Disk 2

2

I = M R 

I = (1/2) M R 

Solid sphere

Thin spherical shell 2

2

I = (2/5) M R 

I = (2/3) M R 

L

L

Thin rod, axis thru center I = (1/12) M L

11/8/2013

2

Thin rod, axis thru end I = (1/3) M L

2

©University of Colorado at Boulder

 

R-13

Appendix 2: Proof of Parallel Axis Theorem.

Consider an object with total mass M and with moment-of-inertia Icm about an axis through the center-of-mass. Let axis A be any axis parallel to that center-of-mass axis. R is the distance  between the axes.

axis through C.M.

axis A

M

R Let’s look at this situation from above the object, looking down along the axes. Let’s place the origin of our xy coordinate system at the location of axis A.

i

ri ri

Axis A



C.M. R

x The position vector of the center-of-mass, relative to the origin, is R. We’re using boldface type for vectors: R  is the position vector. The magnitude of the vector R   (bold) is R (not bold). A mass element mi is a position ri , which can be written as ri = R + ri , where the vector  ri is the ’



 position of mi, relative to the center-of-mass. Recall that the center-of-mass position vector R  is defined by the equation M R

  mi ri . Notice that, if we had chosen the center-of-mass to be i

the location of the origin, then R  would be zero, and ri would be ri , so ’

 m r'  0 i

i

(we’ll

i

need this result in a moment).

11/8/2013

©University of Colorado at Boulder

 

R-14

 m r 



Ok, the moment-of-inertia of the object about the axis A is I

2 i i

. For any position

i

r  R  r' , we have r 2  r  r = (R + r')  (R +r')  R 2  r '2  2R  r' . (Remember: bold is a vector, non-bold is the magnitude of the vector.) So we can write

I 



mi ri2 



i



 

mi (R 2  ri '2  2R  r' i )  

i



mi  R 2 

i



m r '

2

i i

i Icm

M

So

 2R   mi ri ' .

i

0

I  M R 2  ICM . Done!

Appendix 3: Kinetic energy of a rolling wheel. Here we prove that the total kinetic energy of a

rolling wheel (mass M, radius R, center-of-mass speed V) is the translational KE of the center2

2

of-mass motion, KEtrans = (1/2)MV plus the rotational KE about the C.M , KErot = (1/2)Icm . As in Appendix 2, we regard the position vector r of each piece of the wheel as the position R  of the center-of-mass of the wheel plus the position r  of that piece, relative to the center-of-mass. ’

i

ri

ri

origin R



V 

x

The vector equation relating the three vectors is: equation gives

d dt

r

d dt

R

d dt

r  R  r' . Taking the time derivative of this

r' , which is the same as v  V  v' . In words: the velocity

v of each particle of the rolling wheel is the velocity V of the center of the wheel, vector-added

to the velocity v  of the particle relative to the center of the wheel . We showed in Appendix 2 ’

that

 m r'  0 . Taking the time derivative of this equation gives  m v '  0 , a result we i

i

i

i

i

i

will use below.

11/8/2013

©University of Colorado at Boulder

 

R-15

The total kinetic energy of the wheel is KE tot



1

2m v i

2 i

. Now we can write

i

v2  v  v = (V + v')  (V + v')  V2  v '2  2V  v' (remember: bold means vector, non-bold means magnitude.) So, we can rewrite the total KE as

KE tot 

1

2

mi vi2 

i

1



2

i M

that

v '  r ' .

KE tot 

1 2



1



2

mi  V 2 

 i









mi v 'i2   V  





m i v'i  .



i

Now recall

0

So we have

2 MV 

1

m r ' 2 i

i

2 i

1 1  2 2 2     MV I . Done! cm  2 2 

Icm

11/8/2013

©University of Colorado at Boulder

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