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0593_C10_fm  Page 324  Monday, May 6, 2002  2:57 PM





                       324                                                 Dynamics of Mechanical Systems



                                                             t *
                                                             ∫  ⋅
                                                         W = Fv   dt                          (10.2.13)
                                                             0
                             *
                       where t  is the time of action of F. The integrand of Eq. (10.2.13), F • v, is often called the
                       power of F (see Section 10.4).
                        As a second example, consider the work done by gravity on a simple pendulum as it
                       falls from a horizontal position to the vertical equilibrium position as in Figure 10.2.4. Let
                       the pendulum mass be m and let its length be   as shown. The gravity (or weight) force
                       is, then,

                                                          w = mg k                            (10.2.14)

                       where k is a vertically downward directed unit vector as shown in Figure 10.2.4.
                        To apply Eq. (10.2.2), consider that the differential arc vector may be expressed as:


                                                          ds = ldφ n φ                        (10.2.15)

                       where φ measures the angle of the pendulum to the horizontal and n  is a unit vector
                                                                                      φ
                       tangent to the circular arc of the pendulum as shown in Figure 10.2.4. Hence, the work
                       of the weight force is:

                                                   = /
                                                           /
                                                  φπ 2     π 2
                                              W =  ∫  wds  ∫  mg ⋅ n φ dφ
                                                        ⋅
                                                                  l
                                                                k
                                                   φ =0    0
                                                                                              (10.2.16)
                                                     π 2/               π 2
                                                                        /
                                                            d =
                                                =  mgl ∫  cos φφ  mg sin φ  =  mgl
                                                                   l
                                                                        0
                                                      0
                        Observe from the next to last expression of Eq. (10.2.16) that the work done by gravity
                       as the pendulum falls through an arbitrary angle φ is:
                                                           =
                                                         Wmgl sinθ                            (10.2.17)
                        The distance   sinφ may be recognized as the vertical drop h of the pendulum; hence,
                       the gravitational work is:

                                                           W =  mgh                           (10.2.18)


                                                                                P(m)
                                                        k   O
                                                               φ





                                                                            n
                                                                             φ
                       FIGURE 10.2.4
                                                       P(m)
                       A falling pendulum.
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