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                                             b
                                         Fig. 2-33.

         block after each combination of rotations  would also  be different;
         however, in this case, the difference is only a small amount.
              Infinitesimal Rotations. When defining the angular motions of
         a body subjected to three-dimensional  motion, only  rotations which
         are infinitesimally small will be considered. Such rotations can be
         classified as vectors,  since they can  be added  vectorially in any
         manner. To show this, for purposes of simplicity let us consider the
         rigid body  itself to  be a  sphere which is allowed to rotate about its
         central fixed point  O, Fig. 2-34,a.  If we impose two infinitesimal
         rotations dθ  1  + dθ  2  on the body, it is seen that point P moves along the
         path  d ×+θ 1  r  dθ 2 ×r   and ends up at  P'. Had the two successive
         rotations occurred in the order  dθ   2  +  dθ  1 , then the resultant
         displacements of P would have been dθ 2  ×+r  d ×θ 1  r . Since the vector
         cross  product  obeys the  distributive  law, by comparison
          (dθ  1 + dθ  2 )×=r  (dθ  2  +  dθ  1 )×r . Here infinitesimal rotations  dθ are
         vectors, since these quantities have both a magnitude and direction for
         which the order of (vector)  addition is  not important, i.e.,
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