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note 10 rotational motion i sections covered in the text chapter 13 motion is classified as being of one of three types translational rotational or vibrational translational motion is the ...

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                          Note 10                                                                          Rotational Motion I
                                                                                                     Sections Covered in the Text: Chapter 13
                          Motion is classified as being of one of three types:
                          translational, rotational or vibrational.  Translational
                          motion is the motion executed by the center of mass of
                          an object modelled as a particle (Notes 03 and 06). The
                          motion of a baseball hit in a line drive is largely trans-
                          lational. But a baseball can also rotate, so the motion
                          of a baseball can in general possess both translational
                          and  rotational  components.  A  baseball  does  not
                          usually vibrate. We shall study vibrational motion in
                          Note 12.
                               At first thought the motion of a baseball might seem
                          impossibly complicated to describe mathematically.
                          Physics shows, however, that the motion of any object
                          can be separated into its translational and rotational
                          components  and  those  components  solved  for
                          separately. This is possible because translational and                                                                         Figure 10-1. A particle P in a rigid body is located with
                          rotational components of the motion of a rigid body                                                                            respect to O by the polar coordinates (r,θ).
                                                                                                1
                          do not interact with one another.
                               We have already studied a particularly simple form
                          of rotational motion in Note 05: a particle rotating                                                                           Any point P in the object can be located relative to the
                          about a point external to it. This motion is called                                                                            point O with polar coordinates (r,θ). As the object
                          circular motion. Here we survey a few aspects of the                                                                           rotates, P follows a circle of radius r. Every other point
                          rotational motion of a rigid extended body rotating                                                                            in the object also follows a circular path, but a path
                          about a point internal to itself.                                                                                              with a different radius. Let us suppose that in some
                               We begin by laying down the kinematics of a rota-                                                                         elapsed  time  ∆t, P moves from a position on the
                          ting  body  as  we  did  for  a  body  in  translational                                                                       positive x-axis to the point where it is shown in the
                          motion. We derive the kinematic equations of rota-                                                                             figure.  Then  the  subtended  angle  θ  is  called  the
                          tional motion and deduce the relationships between                                                                             angular displacement  of  P  measured  relative  to  the
                          rotational and translational quantities. We introduce                                                                          positive x-axis. Because the object is rigid, the angular
                          the construct of torque.                                                                                                       displacement of every particle in the object is the same
                                                                                                                                                         as the angular displacement of P.
                                                                                                                                                             Angular displacement is measured in the dimen-
                               Angular Speed and Angular Acceleration                                                                                    sionless unit called radian (abbreviated rad) and in the
                                                                                                                                                         following way. The arc length of the circle on which P
                          For convenience we consider a rigid extended object                                                                            moves (the distance travelled by P) is related to the
                          whose mass is confined to a plane and whose trans-                                                                             radius r and angle θ by
                          lational motion is zero (Figure 10-1). We suppose this
                          object  is  rotating  in  a  counterclockwise  direction                                                                                                                       s = rθ ,                                          …[10-1]
                          about  an  axis  perpendicular  to  its  plane  passing
                          through a point O. In the coordinate system of the                                                                                                                                      s
                          figure, this axis can be thought of as the z-axis.                                                                             and therefore                                  θ = .                                              …[10-2]
                               We assume that the object is a rigid, extended body.                                                                                                                               r
                          By this we mean it cannot be modelled as a single
                          particle. It can, however, be modelled (approximately)                                                                         (rad). If s = r then θ = 1 radian. If the object executes
                          as a collection of particles whose positions are fixed                                                                         one complete revolution, then the angular displace-
                          relative to one another. A CD is a rigid body whereas                                                                          ment of P is 2π radians. 2π radians is equivalent to
                          a soap bubble is not.                                                                                                          360˚. If the object executes two revolutions, then its
                                                                                                                                                         angular displacement is 4π radians. By its nature,
                                                                                                                                                         angular displacement is a cumulative quantity.
                          1        But the body must be rigid. Examples of non-rigid bodies
                          whose modes of translation and rotation interact are typically
                          studied in a higher-level course in classical mechanics.
                                                                                                                                                                                                                                                             10-1
                          Note 10
                          We now have the tools we need to define the rota-                                                                                                                                     Δθ            dθ
                          tional equivalents of the translational quantities we                                                                                                             ω≡lim                        =            .                    …[10-5]
                                                                                                                                                                                                      Δt→0 Δt                  dt
                          defined in Note 03. We begin by making Figure 10-1
                          more general (Figure 10-2) by supposing that in some                                                                           We now extend the math to allow for changes in the
                          elapsed time ∆t = tf – ti any arbitrary point P in the                                                                                                                                           3
                                                                                                                                                         instantaneous angular velocity.                                         If the instantaneous
                          object moves from a position i to a position f. These                                                                          angular velocity is changing, then the object is by
                          positions are shown as [A] and [B] in the figure. The                                                                          definition, undergoing an angular acceleration. Let
                          corresponding  angular  positions  are  θi  and  θ f                                                                           the instantaneous angular velocity of the point P at
                          respectively.                                                                                                                  positions i and f be ω  and ω  respectively. The change
                                                                                                                                                                                                       i              f
                                                                                                                                                         in the instantaneous angular velocity divided by the
                                                                                                                                                         corresponding elapsed time is defined as the average
                                                                                                                                                         angular acceleration:
                                                                                                                                                                                                      ωf – ωi                  Δω
                                                                                                                                                                                            α≡                            =              .                 …[10-6]
                                                                                                                                                                                                         t    – t               Δt
                                                                                                                                                                                                           f        i
                                                                                                                                                                                                                                                                –2
                                                                                                                                                         Average angular acceleration has dimension T  and
                                                                                                                                                                       –2
                                                                                                                                                         units s . The limit of the average angular acceleration
                                                                                                                                                         as ∆t → 0 is defined as the instantaneous  angular
                                                                                                                                                         acceleration:
                                                                                                                                                                                                                Δω dω
                                                                                                                                                                                            α≡ lim                        =             .                  …[10-7]
                                                                                                                                                                                                      Δt→0 Δt                   dt
                          Figure 10-2. A more general representation of a rotating                                                                       ω and α are, in fact, vector quantities (pseudo-vectors)
                          body than that shown in Figure 10-1. In some elapsed time                                                                      whose complete vector nature is beyond the scope of
                          ∆t a particle P in the body moves counterclockwise between                                                                                                                                              4
                                                                                                                                                         these notes to describe adequately. But you can find
                          two arbitrary angular positions.                                                                                               the direction of the vectors with the help of the right-
                                                                                                                                                         hand rule as was introduced for the vector cross
                                                                                                                                                         product (Figure 10-3).
                          The angular displacement of P in the interval chosen is
                          defined  as  the  difference  between  the  angular
                          positions that define the interval:
                                                                      ∆θ = θ – θ                                            …[10-3]
                                                                                   f       i
                                      2
                          (rad).            The  angular  displacement  divided  by  the
                          corresponding elapsed time is defined as the average
                          angular velocity:
                                                                        θf –θi                 Δθ
                                                              ω≡                         =             .                    …[10-4]
                                                                          t    –t               Δt
                                                                            f        i
                          Average angular velocity has dimension T–1 and units
                                     –1                       –1
                          rad.s  (or just s  since rad has no dimension). The
                          limit of the average angular velocity as ∆t → 0 is                                                                             Figure  10-3. How to use the right hand rule to find the
                          defined as the instantaneous angular velocity:                                                                                 direction of the vector ω  of a rotating body.
                                                                                                                                                                                                                                 
                                                                                                                                                         3       Of course, in order for the object’s angular velocity to change,
                          2        The  alert  reader  will  notice  the  word  displacement here                                                        the object must be subject to a force applied to it in a special way.
                          implying a vector quantity. Angular displacement is, in fact, a                                                                For the moment we ignore this force, as we did in Notes 02 and 03,
                          vector quantity, or more correctly, a pseudo-vector. This aspect of                                                            and stay within the area of kinematics.
                          rotational motion is somewhat advanced and best left to a second                                                               4       We leave this description to a higher-level course in classical
                          year course in classical mechanics.                                                                                            mechanics.
                          10-2
                                                                                                                            Note 10
                                                                                                           –1            –1
             To find the direction of the ω vector, extend your right     The final angular speed is 10.0 s  or 10.0 rad.s .
             hand, curl your fingers as if you are to grip something      (b) Using the second equation in Table 10-1 we have
             and extend your thumb. Now curl your fingers in the          for the angular displacement
             direction of the angular displacement of the object
             (the direction the object is rotating). Then your thumb              θ =θ +1(ω +ω )t
             points in the direction of the ω vector. By convention,                f     i  2    i     f
             the ω vector is placed on a diagram along the body’s
             axis of rotation. Later in this note we shall see other                   = 0 + 1(0 +10.0rad.s–1)(5.00s)
             uses of the right hand rule.                                                     2
                                                                                       = 25.0 radians.
                           Rotational Kinematics
             As implied in the previous section, a set of kinematic       The number n of revolutions is this number divided
             equations exist for rotational motion just as they do        by the number of radians per revolution (i.e., 2π):
             for translational motion. They have a similar form and
             are derived in a similar fashion. We shall therefore                       n = 25.0(rad) = 3.98 rev.
             just list them (Table 10-1).                                                             
                                                                                             2π rad
                                                                                                      
                                                                                                      
                                                                                                  rev
             Table 10-1. Comparison of translational and rotational kine-
             matic equations.                                             Thus nearly 4 revolutions are required for the wheel
                  Translational Motion        Rotational Motion           to accelerate to the final angular speed of 10.0 s–1.
                      vf = vi + at              ωf = ωi +αt                  € 
                                 1  2                       1   2
                  xf = xi + vit + 2 at      θf =θi +ωit + 2αt             Relations exist between the angular and tangential
                 x = x + 1(v +v )t         θ =θ +1(ω +ω )t                speeds of a particle in a rotating rigid body, and bet-
                   f    i  2   i   f         f    i   2   i    f          ween the angular and tangential accelerations. Since
                 v2 = v2 + 2a(x – x )      ω2 = ω2 + 2α(θ –θ )            these relations are useful in solving rotational motion
                  f    i        f    i        f    i        f    i        problems we consider them next.
             Problems in rotational kinematics can be solved much
             like problems in translational kinematics. Assuming                 Relations Between Rotational and
             you have memorized the translational equations and
             know  the  rotational  equivalents,  you  can  easily                      Translational Variables
             reconstruct the rotational equations. Let us consider        Suppose that a rigid extended body rotates about an
             an example.                                                  axis that passes through an internal point O as shown
                                                                          in Figure 10-4. Consider a point P in this body.
             Example Problem 10-1
             A Problem in Rotational Kinematics
             Starting from rest a wheel is rotated with a constant
             angular acceleration of 2.00 rad.s–2 for 5.00 s. (a) What
             is the final angular speed of the wheel? (b) How many
             complete revolutions does the wheel execute in the
             elapsed time of 5.00 s?
             Solution:
             (a) Using the first equation in Table 10-1 we have for
             the final angular speed
                     ω =ω +αt=0+(2.00s–2)(5.00s)
                        f     i
                          = 10.0 s–1.
                                                                               Figure 10-4. A particle P in a rotating rigid body.
                                                                                                                           10-3
             Note 10
             The magnitude of the tangential velocity of P is, from          Table 10-2. Relationships between the magnitudes of trans-
             eq[10-1],                                                       lational and rotational variables.
                                       ds     dθ                                Translational     Rotational         Relationship
                                  v =     = r     ,                                   x                θ               x =θr
                                       dt      dt
                                                                                      v               ω                v =ωr
             since r is constant. Thus using the definition of ω in                   a                α           a =αr =ω2r
             eq[10-5]
                                     v =rω .                  …[10-8]        Let us consider an example.
             The tangential acceleration of P is, using eq[10-8],
                                       dv      dω                            Example Problem 10-2
                                 at =      =r      ,                         Tangential and Angular Speeds
                                       dt       dt
             again since r is constant, or using the definition of α in      A bicycle wheel of diameter 1.00 m spins freely on its
                                                                                                                    –1
             eq[10-7],                                                       axis at an angular speed of 2.00 rad.s . (a) What is the
                                     at = rα.                 …[10-9]        tangential speed of a point on the rim of the wheel?
                                                                             (b) What is the tangential speed of a point halfway
             Now since P is moving in a circle it is undergoing a            between the axis and the rim?
             centripetal  acceleration.  The  magnitude  of  this
             centripetal or radial component of the acceleration is          Solution:
                                                                             (a) Using eq[10-8] the tangential speed of a point on
                                        v2                                   the rim of the wheel is
                                  a =      =rω2.
                                    c    r       z
                                                                                             1.00m
                                                                                                                –1             –1
             using eq[10-8].                                                    v =rω =               (2.00rad.s ) =1.00 m.s .
                                                                                               2    
                The relationship between tangential and radial com-
             ponents of the acceleration of P can be seen with the
             help of Figure 10-5. The total acceleration of P is the         (b) A point halfway between axis and rim will have a
             sum of the a  and  a vectors. The complete vector               tangential speed one half of this value, or
                             t       r
             nature of a and a  is beyond the scope of these notes
                         t      c                                                                 v = 0.50 m.s–1.
             to describe. The relationships between the magnitudes
             of these quantities are summarized in Table 10-2.
                                                                             Clearly, the further a point on the wheel is from the
                                                                             axis of rotation the greater is its tangential speed.
                                                                             Though the  two  points  have  different  tangential
                                                                             speeds they have the same angular speed.
                                                                             We stated in Note 07 without proof that the centre of
                                                                             mass of a rigid body can be taken to be the body’s
                                                                             geometric centre. We are now ready to extend the idea
                                                                             of the centre of mass to a system of discrete bodies,
                                                                             and  to  define  the  centre  of  mass  in  a  proper
                                                                             mathematical fashion.
             Figure 10-5. The resultant acceleration of any particle P in a
             rotating rigid body is the vector sum of the tangential and
             radial acceleration vectors.
             10-4
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...Note rotational motion i sections covered in the text chapter is classified as being of one three types translational or vibrational executed by center mass an object modelled a particle notes and baseball hit line drive largely trans lational but can also rotate so general possess both components does not usually vibrate we shall study at first thought might seem impossibly complicated to describe mathematically physics shows however that any be separated into its those solved for separately this possible because figure p rigid body located with respect o polar coordinates r do interact another have already studied particularly simple form rotating point relative about external it called circular here survey few aspects rotates follows circle radius every other extended path internal itself different let us suppose some begin laying down kinematics rota elapsed time t moves from position on ting did positive x axis where shown derive kinematic equations then subtended angle tional ded...

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