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0593_C07_fm  Page 220  Monday, May 6, 2002  2:42 PM





                       220                                                 Dynamics of Mechanical Systems


                        Let P  and P  be a typical pair of particles taken from a set S of particles for which Π is
                             1
                                   2
                       a plane of symmetry. Then, from Eq. (7.7.2) we see that the contributions of P  and P  to
                                                                                                   2
                                                                                            1
                       the second moment of S relative to O for the direction of n are represented by:
                                                          ×
                                                                        ×
                                             I SO  =  m p ×( n p ) +  m p ×( n p ) +K
                                              n      1       1     2       2
                                                       +
                                                =  m( OP h n) ×[ n ×( OQ h n)]
                                                                      +
                                                                                               (7.9.36)
                                                                       −
                                                        −
                                                 + m( OQ h n) ×[ n ×( OQ h n)] +K
                                                        2
                                                = 2 m OQ n +K
                       where the last equality follows from expanding the triple products of the previous equality
                       and where the terms not written in Eq. (7.9.36) represent the contributions to I  SO  from the
                                                                                            a
                       other pairs of particles of S. However, by analyses identical to those shown in Eq. (7.9.36),
                       these contributions to  I  SO  are also parallel to n. Therefore,  I SO  is parallel to n, and thus
                                            a                                n
                       n is a principal unit vector of S for O.
                        A specialization of these ideas occurs if the system of particles all lie in the same plane,
                       as with a planar body. A unit vector normal to the plane is then a principal unit vector.
                        There are other ways of determining principal unit vectors without solving Eqs. (7.7.10)
                       and (7.7.12). For homogeneous bodies occupying common geometric shapes, we can
                       simply refer to a table of results as in Appendix II. We can also make use of a number of
                       theorems for principal unit vectors stated here, but without proof (see References 7.1 and
                       7.2 for additional information). If a line is parallel to a principal unit vector for a given
                       reference point, then that line is called a principal axis for that reference point. A principal
                       axis for the mass center as a reference point is called a central principal axis. Then, it can
                       be shown that:

                          1. If a principal axis for a reference point other than the mass center also passes
                             through the mass center, then it is also a central principal axis.
                          2. Mutually perpendicular principal axes that include a central principal axis for
                             any point on the central principal axis are parallel to mutually perpendicular
                             central principal axes.
                          3. A central principal axis is a principal axis for each of its points.

                        Finally, regarding the question as to whether the procedures of the example of the
                       previous section will always produce principal unit vectors and principal moments of
                       inertia, the answer is yes, but as seen above there may exist simpler procedures for any
                       given problem. That is, a principal unit vector may often be identified by inspection —
                       for example, as being normal to a plane of symmetry. In this case, the task of solving a
                       cubic equation may be reduced to that of solving a quadratic equation.
                        To illustrate the procedure, suppose that a principal unit vector found by inspection is
                       called n . Then, let n  and n  be unit vectors perpendicular to n  and also perpendicular
                                                2
                              3
                                                                                3
                                         1
                       to each other so that n , n , and n  form a mutually perpendicular set. Then, because n 3
                                           1
                                              2
                                                     3
                       is a principal unit vector, the inertia dyadic I expressed in terms of n , n , and n  has a
                                                                                      1
                                                                                                3
                                                                                         2
                       matrix of components in the form:
                                                          I   I     0  
                                                           11  12     
                                                     I =  I    I     0                         (7.9.37)
                                                      ij   21  22     
                                                           0  0   I  
                                                                     33
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