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0593_C08_fm  Page 267  Monday, May 6, 2002  2:45 PM





                       Principles of Dynamics: Newton’s Laws and d’Alembert’s Principle            267











                       FIGURE 8.12.4
                       An incorrect free-body diagram of the
                       rotating rod.
















                       FIGURE 8.13.1
                       A circular disk rolling on a horizontal
                       surface S.






                       8.13 The Rolling Circular Disk

                       For another illustration of a body with nonplanar motion, consider again the rolling
                       circular disk (or rolling coin) as discussed in Section 4.12. That is, let D be a circular disk
                       with mass m and radius r rolling on a “perfectly rough” flat horizontal surface S as in
                       Figure 8.13.1. Let the orientation of D be defined by the roll, lean, and turning angles ψ,
                       θ, and φ, as shown. Let G be the mass center of D, and let C be the contact point of D with S.
                        When we studied the kinematics of D in Section 4.12, we discovered that the requirement
                       that D rolls on S led to the following expressions for the velocity and acceleration of G
                       and the angular velocity and angular acceleration of D in an inertia frame R (in which S
                       is fixed) (see Eqs. (4.12.2), (4.12.3), (4.12.7), and (4.12.8)):

                                                    v = ( r ˙ ψφθ n )  − rθ ˙ n                (8.13.1)
                                                            ˙
                                                          + sin
                                                                   1    2
                                          + sinθ
                                                                                 θ
                                   a = ( r ˙˙ ψ φ  + φθ2 ˙ ˙  cosθ n )  1 ( θ ψφ cosθ + φ ˙ 2 sin cosθ n )  2
                                                             +− + ˙ ˙
                                           ˙˙
                                                                 ˙˙
                                                              r
                                                 −
                                           ˙ ˙
                                      +− ( r ψφθ φ ˙ 2 sin θ − θ ˙ 2  n )                      (8.13.2)
                                                        2
                                             sin
                                                               3
                                                   ˙
                                                         ˙
                                                ωω= θn  +( ψ + sinφ ˙  ) θ n  + cosφ ˙  θn     (8.13.3)
                                                     1             2        3
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