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0593_C14_fm  Page 485  Tuesday, May 7, 2002  6:56 AM





                       Stability                                                                   485


                                   2
                       (specifically, Ω  < g/r), there are only two equilibrium positions: θ = θ  = 0 and θ = θ  = π,
                                                                                    1
                                                                                                 2
                       with θ = θ  = 0 being stable (see Eq. (14.3.7)) and θ = θ  = π being unstable (see Eq. (14.3.10)).
                               1
                                                                     2
                                                         2
                       For fast tube rotation (specifically,  Ω  >  g/r), there are three equilibrium positions:
                                                             2
                                                       –1
                       θ = θ  = 0, θ = θ  = π, and θ = θ  = cos (g/rΩ ), with θ = θ  = 0 and θ = θ  = π being unstable
                                    2
                           1
                                                 3
                                                                        1
                                                                                     2
                       (see Eqs. (14.3.7) and (14.3.10)) and θ = θ  = cos (g/rΩ ) being stable (see Eq. (14.3.16)).
                                                                  –1
                                                                        2
                                                            3
                       That is, the third equilibrium position does not exist unless the tube rotation is such that
                        2
                       Ω  > g/r, but if it does exist, it is stable.
                       14.4 A Freely Rotating Body
                       Consider next an arbitrarily shaped body B that is thrown into the air, rotating about one
                       of its central principal axes of inertia. Our objective is to explore the stability of that motion;
                       that is, will the body continue to rotate about the principal inertia axis or will it be unstable,
                       wobbling away from the axis?
                        To answer this question, consider a free-body diagram of B as in Figure 14.4.1, where
                       G is the mass center of B; m is the mass of B; k is a vertical unit vector; F  and T  are the
                                                                                               *
                                                                                        *
                       inertia force and couple torque, respectively, of a force system equivalent to the inertia
                       forces on B; –mgk is equivalent to the gravitational forces on B, with g being the gravity
                       constant; and R is an inertial reference frame in which B moves. In the free-body diagram,
                       we have neglected air resistance; thus, the gravitational (or weight) force –mgk is the only
                       applied (or active) force on B.
                        From Eqs. (7.12.1) and (7.12.8), we recall that the inertia force F  and couple torque T *
                                                                                  *
                       may be expressed as:
                                                                           I⋅ )
                                                                    α
                                              F =−m  a and   T =− ⋅ −αωω × ( ωω                (14.4.1)
                                                                  I
                                                              *
                                               *
                       where  a is the acceleration of  G in  R;  ωω ωω and  αα αα are the angular velocity and angular
                       acceleration, respectively, of B in R; and I is the central inertia dyadic of B (see Sections
                       7.4 to 7.9).
                        From the free-body diagram we then have:
                                                              +
                                                        −mgkF   *  = 0                         (14.4.2)

                       and

                                                            T = 0                              (14.4.3)
                                                             *


                                                                                       B
                                                                     F  *
                                                             k
                                                                                             T *
                                                                           G


                                                                            -mgk
                       FIGURE 14.4.1
                       Free-body diagram of freely rotating body.
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