Page 516 - Bird R.B. Transport phenomena
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496  Chapter 16  Energy  Transport by Radiation

                                                                           Fig. 16.3-2.  Comparison of  the emit-
                                                                           ted radiation from  black, gray, and
                                                                           real  surfaces.

                                                Planck's law (black body)

                                                    A typical real surface
                                                        Gray body with e -  1 /3










                                                                  7
                              an empiricism that fitted  the available  data.  However,  before  the end  of  the year, 8  Planck
                              succeeded  in deriving the equation, but  at  the expense  of  introducing  the radical  notion
                              of the quantization of energy, an idea that was  met with  little enthusiasm. Planck  himself
                              had misgivings, as clearly  stated in his textbook. 9  In a letter in 1931, he wrote: "..  . what I
                              did  can be described  as an act of desperation....  I had been wrestling  unsuccessfully  for
                              six  years...  with  the problem  of  equilibrium  between  radiation and  matter, and  I knew
                                                                         .
                              that  the problem  was  of  fundamental  importance .."  Then Planck went  on  to say  that
                              he was  "ready  to sacrifice  every  one of my previous  convictions about physical  laws"  ex-
                              cept  for  the  first  and  second  laws  of  thermodynamics. 10  Planck's  radical  proposal  ush-
                              ered  in  a  new  and  exciting  era  of  physics,  and  quantum  mechanics  penetrated  into
                              chemistry and other fields  in the twentieth century.


          EXAMPLE   16.3-1    For  approximate  calculations,  the  sun  may  be  considered  a  black  body,  emitting  radiation
                              with a maximum intensity at Л = 0.5 microns  (5000 A). With  this information, estimate  (a) the
         Temperature  and     surface  temperature of the sun, and (b) the emitted heat flux  at the sun's  surface.
         Radiant-Energy
         Emission  of  the  Sun  SOLUTION
                              (a)  From Wien's  displacement law,  Eq. 16.3-12,

                                                    0.2884  0.2884 cm К
                                                T =                4   =  5760K  = 10,400 R       (16.3-13)
                                                       ax   0.5X10" cm
                              (b)  From the Stefan-Boltzmann  law, Eq. 16.2-10,
                                                                          8
                                                     cjf  = aT 4  = (0.1712  X 10~ )(10,400) 4
                                                                      7
                                                             =  2.0 X  10 Btu/hr-ft  2            (16.3-14)





                                  7  O. Lummer and  E. Pringsheim, Wied. Ann.,  63, 396  (1897); Ann.  der Physik, 3,159  (1900).
                                  8  M. Planck, Verhandl.  d. deutsch.  physik.  Ges., 2, 202 and 237 (1900); Ann.  Phys., 4, 553-563,  564-566
                              (1901).
                                  9  M. Planck, The Theory of Heat Radiation, Dover, New  York  (1991), English  translation of  Vorlesungen
                              iiber die Theorie der  Warmestrahlung  (1913), p. 154.
                                  10  A. Hermann, The Genesis of Quantum  Theory, MIT Press  (1971), pp. 23-24.
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