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0593_C08_fm  Page 251  Monday, May 6, 2002  2:45 PM





                       Principles of Dynamics: Newton’s Laws and d’Alembert’s Principle            251






                                                                                      F*
                                                                                           T*


                                                                               G



                                                                               W

                       FIGURE 8.7.1                                FIGURE 8.7.2
                       A body B moving as a projectile.            A free-body diagram of projectile B.






                       8.7  Projectile Motion
                       To illustrate the use of Eqs. (8.6.5) and (8.6.6), consider a body thrown into the air as a
                       projectile as in Figure 8.7.1. Then, the only applied forces on B are due to gravity, which
                       can be represented by the single weight force W passing through G as:


                                                         W =−MgN                                (8.7.1)
                                                                   3
                       where N  is the vertical unit vector shown in Figure 8.7.1. Figure 8.7.2 shows a free-body
                              3
                       diagram of B. Using d’Alembert’s principle, the governing equations of motion of B are,
                       then,


                                                          W + F *  = 0                          (8.7.2)

                       and

                                                             *
                                                            T = 0                               (8.7.3)
                       or

                                                          a =−  gN                              (8.7.4)
                                                         RG
                                                                   3
                       and

                                                        T = T = T =  0                          (8.7.5)
                                                         1   2   3

                        Suppose the acceleration of G is expressed in the form:

                                                     RG
                                                          xN + ˙˙
                                                      a = ˙˙   yN + ˙˙                          (8.7.6)
                                                                     zN
                                                             1    2    3
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