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110 2. Introductory applications



               (a) Write  your solution,  and the  differential  equation, in  terms of the non-
                  dimensional variables                        and introduce the
                  parameter           Suppose that the limit of interest is   (which
                  you may  care to  interpret); find  the first two terms of an  asymptotic ex-
                  pansion, valid for     (in the  form         directly from the
                  governing equation. (You  should compare  this with the  expansion of the
                  exact solution.) From your results, find approximations to the time to reach
                  the maximum height, the value of this height and the time to return to the
                  point of projection.
               (b) A better model,  for motion through an atmosphere, is represented by the
                  equation





                  where        is  a constant. (This is  only a  rather crude  model for  air
                  resistance,  but it has the considerable advantage  that it is  valid for  both
                       and      Non-dimensionalise this equation as in (a), and then write
                                                where                  Repeat
                  all the calculations in (a).
               (c) Finally, in  the  special  case  (i.e.  the escape speed), find
                  the first term in an asymptotic expansion valid as   Now  find the
                  equation for the second term and a particular integral of it. On the assump-
                  tion that the rest of the solution contributes only an exponentially decaying
                  solution, show that your expansion breaks down at large distances; rescale
                  and write down—do not solve—the  equation valid in this new region.
          Q2.28 Earth-moon-spaceship (1D). In this simple model for the passage of a spaceship
               moving from the Earth to our moon, we assume that both these objects are fixed
               in our chosen coordinate system, and that the trajectory is along the straight line
               joining the two centres of mass. (More complete and accurate models will be
               discussed in later exercises.) We take x(t) to be the distance measured along this
               line from the Earth, and then Newton’s Law of Gravitation gives the equation
               of motion  as





               where m  is the mass  of the spaceship,   and   the masses  of the Earth
               and Moon, respectively, G is the  universal gravitational  constant and d the
               distance between the mass centres. Non-dimensionalise this equation, using d
               as the distance scale and           as the time scale, to give the non-
               dimensional version of the equation (x and t now non-dimensional) as
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