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112                                                      Chapters

           Table 3.3.1 Continued

           hi^W)                                                       (3.3.13)

           hi,2 = W)                                                   (3.3.14)
                                                                       (3.3.15)

                                                                      (3.3.16)

           h 2L>, =  f(T 2)                                           (3.3.17)
           h 2L,2 = f(T 2)                                            (3.3.18)

           Variables
                               m
           y 2v,i - y 2v, 2  • y 2L,i - y 2L, 2 • 2v  - rn 2L - T 2 - K 2jl  - K 2;2 - h t -  hi_i - h 1;2 - h 2V - h 2v,i - h 2V>2 - h 2L

           Degrees of Freedom

           F=18-18 = 0


           Next  the  equations  that  we  can  write  are  for  calculating  system  properties.  Be-
           cause  equilibrium is  assumed,  the rate  equations and,  therefore,  the transport  and
           transfer properties are of no concern. In  general, the thermodynamic properties of
           mixtures will  depend  on temperature, pressure,  and composition,  we will  assume
           that the mixture is an ideal solution to simplify  the computation of thermodynamic
           properties.  Thus, we can write the enthalpies of the mixtures as mole fraction  av-
           erages of the pure component enthalpies, without an enthalpy of mixing term. We
           can  also  write  the  phase  equilibrium  relations  as  functions  of  temperature  and
           pressure  only  and  not  composition.  The  pure  component  enthalpies  of  liquids
           generally  do  not  depend  strongly  on  pressure,  but  there  may  be  some  effect  of
           pressure on the vapor-phase enthalpy.  We will neglect this effect  for simplicity.
                The  next  step  in the problem  solving  format  is to prime  the  specified  vari-
           ables in the  equations  listed  in  Table  3.3.1. Next,  list  the unknown variables  and
           calculate the degrees of freedom.  The  degrees of freedom  are zero, and therefore,
           a  solution  is  possible.  Now  that  the  problem  is  completely  formulated,  the  next
           step is to outline a solution procedure.
                The  solution of the equations listed  in Table 3.3.1 requires an iterative pro-
           cedure.  Thus,  it is good strategy to examine the variables to determine if there are
           limits  on  their  values.  For  example,  the  mole  fractions  of  the  components  will
           vary from zero to one. This fact greatly simplifies the solution procedure. Also, the
           final  flash temperature will lie somewhere between the bubble and dew-point  tem-
           peratures.  The  bubble-point  temperature  is  that  temperature  at  which  the  first




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