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0593_C04*_fm  Page 109  Monday, May 6, 2002  2:06 PM





                       Kinematics of a Rigid Body                                                  109


                       to know the derivative of the n  in S. These derivatives may be obtained by noting that
                                                   i
                       the n  are fixed in R  and by using Eq. (4.5.2). That is,
                                        2
                           i
                                                  S    dt= ωω R 2  ×  i (  )
                                                          S
                                                                      ,,
                                                   dn          n   i = 12 3                    (4.12.4)
                                                     i
                       From the configuration graph of Figure 4.12.2, we see that  ωω  R 2  is:
                                                                            S
                                                    ωω  = θn  +  s φ n  +  c φ n               (4.12.5)
                                                   S  R 2  ˙  ˙      ˙
                                                            1   θ  2  θ  3
                       Hence, the derivatives in S of the n  are:
                                                      i
                                          S    dt = φ ˙ c n − φ ˙  S  dt = −φ ˙ c n + θ ˙
                                           dn             s n ,   dn            n
                                              1      θ  2  θ  3   2        θ  1  3
                                                                                               (4.12.6)
                                                     S        ˙     ˙
                                                      dn  dt = φ s n − θ n
                                                         3      θ  1   2
                       Using these results the angular acceleration of D in S and the acceleration of G in S are
                       found to be:

                                                      − ˙ ˙
                                               αα= ( θψφψ φ          s + θφ c ) n 2
                                                                  +
                                              S  D  ˙˙        +(    ˙˙  ˙ ˙
                                                                 ˙˙
                                                          c ) n
                                                                     θ
                                                          θ
                                                                           θ
                                                             1
                                                                                               (4.12.7)
                                                        ˙˙
                                                            ˙ ˙
                                                                  ˙ ˙
                                                                  ψθ
                                                      +( φ c − φθ s + ) n 3
                                                          θ
                                                               θ
                       and
                                                                   ˙˙
                                                         ˙ ˙
                                                                 r( θ ψφ
                                                    s +
                                          a =
                                                 +
                                                   ˙˙
                                                ˙˙
                                         SG   r( ψφφθ     c n )  1 +− + ˙ ˙ c + φ ˙ 2 s c n )  2
                                                       2
                                                                         θ
                                                                              θ θ
                                                     θ
                                                           θ
                                                                s − )
                                                           s −
                                                      r +− ( ψφφ ˙ 22 θ  θ ˙ 2  n  3           (4.12.8)
                                                         ˙ ˙
                                                            θ
                        Finally, consider the special case of straight-line rolling of a disk or wheel as depicted
                       in Figure 4.11.4. As before, let the disk have radius r, center G, and contact point C. Let P
                       be a point on the rim of D such that GP is perpendicular to GC, as in Figure 4.11.4. We
                       can obtain expressions for the kinematics of D and G directly from the expressions of Eqs.
                       (4.12.2), (4.12.3), (4.2.7), and (4.12.8) by setting θ and φ equal to zero. That is:
                                                    S  D       S  G  =
                                                     ωω = ˙ ψn  ,  V  r ˙ ψn
                                                             2          1
                                                                                               (4.12.9)
                                                    S  D      S G  =
                                                     αα = ˙˙ ψn  ,  a  r ˙˙ ψn
                                                             2         1
                       Observe the relative simplicity of these expressions. Indeed, these expressions may be
                       recognized as those learned in elementary mechanics.
                        Finally, using Eqs. (4.11.1), (4.11.5), (4.9.4), and (4.9.6), we can evaluate the velocity and
                       acceleration of P and C. The results are:
                                                 rψ
                                                      rψ
                                                                  ˙˙
                                                             p
                                                                 r − ˙
                                              P
                                            V = ˙  n − ˙  n ,  a = ( ψ  rψ  2  n )  − r ˙˙ ψ n
                                                    1     3               1     3
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