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72                                                                                     PHYSICS


                                                                           Example 4.3 A motorboat is racing
                                                                          t
                                                                           towards north at 25 km/h and the water
                                                                           current in that region is 10 km/h in the
                                                                           direction of 60° east of south. Find the
                                                                           resultant velocity of the boat.

                                                                        Answer   The vector v  representing the velocity
                                                                                             b
                                                                        of the motorboat and the vector v representing
                                          Fig. 4.10                                                      c
                                                                        the water current are shown in Fig. 4.11 in
                       Answer  Let OP and OQ represent the two vectors  directions specified by the problem. Using the
                       A and B making an angle θ  (Fig. 4.10).  Then,   parallelogram method of addition, the resultant
                       using the parallelogram method of vector         R  is obtained in the direction shown in the
                       addition, OS represents the resultant vector R :  figure.
                                    R = A + B
                       SN is normal to OP and PM is normal to OS.
                       From the geometry of the figure,
                                      2
                                2
                             OS  = ON  + SN 2
                       but   ON = OP + PN = A + B cos θ
                          SN = B sin θ
                             OS  = (A + B cos θ)  + (B sin θ) 2
                                               2
                                2
                       or,   R  = A  + B  + 2AB  cos θ
                              2
                                   2
                                       2
                                      2
                                 2
                          R =   A +  B +  2AB cos  θ          (4.24a)
                       In ∆ OSN,   SN = OS sinα = R sinα,  and
                       in ∆ PSN,   SN = PS sin θ = B sin θ
                       Therefore,   R sin α  = B sin θ
                               R      B
                       or,         =                          (4.24b)
                              sin θ  sin α
                                                                                           Fig. 4.11
                       Similarly,
                                PM = A  sin α  = B  sin β
                                                                        We can obtain the magnitude of R using the Law
                               A      B
                       or,         =                          (4.24c)   of cosine :
                              sin β  sin α
                                                                                 2
                                                                                      2
                       Combining Eqs. (4.24b) and (4.24c), we get          R =  v +  v +  2 v v cos120 o
                                                                                      c
                                                                                           b c
                                                                                 b
                               R      A      B
                                                                                                (
                                                                                        ×
                                                                                            ×
                                                                              2
                                                                                   2
                                   =      =                   (4.24d)    = 25 +  10 + 2 25 10 -1/2) ≅    22 km/h
                              sin θ  sin β  sin α
                                                                        To obtain the direction, we apply the Law of sines
                       Using Eq. (4.24d), we get:
                                                                                R     v c            v
                                    B                                              =        or, sin  φ =  c  sin  θ
                                 sin α =  sin θ               (4.24e)         sin θ  sin φ            R
                                    R
                       where R is given by Eq. (4.24a).                         10 sin120     10 3
                                                                                  ×
                                                                              =            =        ≅  0.397
                                                                                              ×
                       or, tanα =   SN    =   B sinθ           (4.24f)             21.8      2 21.8
                                 OP +  PN   A +  B cosθ
                                                                              φ ≅  23.4                             t
                       Equation (4.24a) gives the magnitude of the
                       resultant and Eqs. (4.24e) and (4.24f) its direction.  4.7  MOTION IN A PLANE
                       Equation (4.24a) is known as the Law of cosines  In this section we shall see how to describe
                       and Eq. (4.24d) as the Law of sines.                    t  motion in two dimensions using vectors.
                                                               2018-19
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