Page 244 - Advanced Thermodynamics for Engineers, Second Edition
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232    CHAPTER 10 THERMODYNAMICS OF COMBUSTION




                Hence T P < 2800 K.
                Use T P ¼ 2700 K.




                        Constituent    CO 2         CO           H 2 O        N 2

                           h 2700     144,256.1    91,070.2    118,376.1    90,326.0
                            n           3.5          2.5          3           23.5
                            nh        504,896.3   227,675.4    355,128.2    2,122,661




                                            H P ðT P Þ ¼ 3210360:9kJ:
                Interpolate linearly
                                          3313406:9   3210360:9
                                                                100 ¼ 2776:8K:
                               T P ¼ 2700 þ
                                          3344558:7   3210360:9

                        Constituent     CO 2          CO         H 2 O        N 2

                           h 2777     149,011.4     93,936.1    122,512.5   93,181.1
                            n           3.5           2.5          3          23.5
                            nh         521,540     234,840.3    367,537.5   2,189,757

                                            H P ðT P Þ¼ 3313674:8kJ:

                Hence the equations balance within 0.020%.
                The pressure at the end of combustion is the same as that at the end of compression i.e.
             p 3 ¼ 44.31 bar. Hence the volume at the end of combustion, V 3 , is given by

                                     n P <T P  p 1    32:5   2777   1
                                                                         V 1
                                V 3 ¼            V 1 ¼
                                     n R <T 1  p 3    30:75   298  44:31
                                                    ¼ 0:2223 V 1 :

             10.7 CONCLUDING REMARKS

             A consistent method of analysing combustion has been introduced. This is suitable for use with all the
             phenomena encountered in combustion, including weak and rich mixtures, incomplete combustion,
             heat and work transfer, dissociation and rate kinetics. The method which is soundly based on the First
             Law of Thermodynamics ensures that energy is conserved. While the approach seems cumbersome for
             hand calculations it is easily implemented in computer programs.
                A large number of examples of different combustion situations have been presented.
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