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0593_C14_fm  Page 490  Tuesday, May 7, 2002  6:56 AM





                       490                                                 Dynamics of Mechanical Systems


                                                               3
                       Thus, if the angular speed of D exceeds  gr , D will remain erect and continue to roll
                                                                            3
                       in a straight line. If the angular speed of D is less than  gr , the motion is unstable. D
                       will wobble and eventually fall.

                       Case 2: Rolling in a Circle
                                                                                      φ
                                                                                      ˙
                       Next, suppose D is rolling in a circle with uniform speed such that θ,  , and  ˙ ψ  are (see
                       Figure 14.5.1):

                                                               ˙
                                                      =
                                                            ˙
                                                                   ˙
                                                    θθ ,   φ =  φ ,  ψ = ˙ ψ                  (14.5.14)
                                                        0       0       0
                       By inspection of the governing equations, we see that Eqs. (14.5.2) and (14.5.3) are then
                       identically satisfied and that Eq. (14.5.1) becomes:
                                          ( 4gr)sinθ 0 + ψ φ  cosθ 0 + 5φ 2 0 sinθ 0 cosθ 0  =  0  (14.5.15)
                                                      6 ˙ ˙
                                                         0 0
                        Equation (14.5.15) provides a relationship between  θ ,  φ ˙  0 , and  ˙ ψ 0 . By inspection of
                                                                         0
                       Figure 14.5.1 we see that if  φ ˙  0  and  ˙ ψ 0  are positive, then Eq. (14.5.15) requires that θ  be
                                                                                                  0
                       negative. That is, the disk will lean toward the interior of the circle on which it rolls.
                        To test the stability of this motion, let the disk encounter a small disturbance such that
                          ˙
                         φ
                       θ,  , and  ˙ ψ  have the forms:
                                                =
                                                          ˙
                                              θθ +   θ ,  φ = φ +  φ ,  ψ = ˙  ψ  *           (14.5.16)
                                                             ˙
                                                                 * ˙
                                                                        ψ + ˙
                                                                     ˙
                                                      *
                                                   0          0          0
                       where, as before, the quantities with the ( ) are small. Then, sinθ and cosθ are:
                                                            *
                                               sinθ = (     θ *  sinθ + θ  * cosθ
                                                     sin θ + ) =
                                                         0          0        0                (14.5.17)
                       and
                                                        (
                                                            θ
                                               cosθ =  cos θ + ) =  cosθ − θ * sinθ 0         (14.5.18)
                                                             *
                                                                     0
                                                         0
                        By substituting from Eqs. (14.5.16), (14.5.17), and (14.5.18) into Eqs. (14.5.1), (14.5.2), and
                       (14.5.3) and by neglecting quadratic (second) and higher order terms in the ( ) terms we
                                                                                            *
                       obtain:
                                     ( 4gr)sinθ 0 + ψ φ  cosθ 0 + 5φ 2 ˙  0 sinθ 0 cosθ 0 ( 4gr) cosθ 0
                                                                                 θ
                                                 6 ˙ ˙
                                                                          +
                                                                                  *
                                                   0 0
                                     − 5θ  + ψ φ  cosθ  + ψ φ  cosθ  − ψ φ θ * sinθ           (14.5.19)
                                                                   6 ˙ ˙
                                                       6 ˙ ˙
                                                         *
                                       ˙˙*
                                           6 ˙ ˙ *
                                             0      0      0    0    0 0      0
                                                          2 ˙
                                     + 10φφ  sinθ  cosθ  + 5φ θ *  cos θ  − 5φ θ sin θ=  0
                                                                      2 ˙
                                                                            2
                                                               2
                                         ˙˙ *
                                                                        * *
                                         0      0    0    0      0    0       0
                                                  ψ +
                                                       ˙˙*
                                                 3 ˙˙ *  3φ  sinθ + 5φ θ  cosθ =  0           (14.5.20)
                                                                 ˙ ˙ *
                                                             0   0      0
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