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26         SAMAGRA  TILAK - 2  •  THE  ARCTIC  HOME

          of summer and winter would be the longest, when the  eccentricity
          of the  earth is  at its  maximum  and  according  as  the  winter  and
          summer  occur  at  the  points  of  perihelion  or  aphelion.  It has
          been found  that this difference is  equal to 33  days at  the highest,
          and that at the present day it is about 7i  days. Thus  if the winter
          in  the  northern  hemisphere  occurs  when  the  earth  is  at P  in  its
          orbit  and  the  eccentricity  is  at  its  maximum,  the  winter  will  be
          shorter  by  33  days  than  the  summer  of the  time.  But  this  posi-
          tion  will  be  altered  after 10,500 years  when the  winter, occurring
          at A,  will,  in  its  turn,  be longer than the  corresponding  summer
          by the same length of time, viz.  33  days.
              Now,  since  the  earth describes  equal  areas  in  equal  times  in
          its orbit, Herschel supposed that in spite of the difference between
          the duration of summer and winter noticed above, the whole earth
          received  equal  amount  of heat  while  passing  from  one  equinox
          to  another, the "  inequality in the intensities  of solar radiation in
          the  two  intervals  being  precisely  compensated  by  the  opposite
          inequality in the duration of the intervals themselves.  "  Accepting
          this  statement  Dr.  Croll  understated  his  case  to  a  certain  extent.
          But  Sir  Robert  Ball,  formerly  the  Astronomer  Royal  of Ireland,
          in  his  recent work On  the  Cause of an  Ice  Age has demonstrated,
          by  mathematical  calculation,  that  the  above  supposition  is
          erroneous,  and  that the  total  amount  of heat  received  from  the
          sun  by  each  hemisphere  in  summer  and  winter  varies  as  the
          obliquity  of the  earth  or the  inclination  of its  axis  to  the  eclip-
          tic,  but  is  practically  independent  of  the  eccentricity  of the
          earth's  orbit.  Taking the total  sun-heat received in a year by each
          hemisphere to be 365 units,  or on an average one  unit a day,  and
          taking  the obliquity  to be  23°  27',  Sir Robert  Ball has  calculated
          that each hemisphere would receive 229  of these heat-units during
           summer  and  only  136  during winter, whatever the eccentricity of
           the  earth may be.  But though these figures  are not  affected by the
          eccentricity of the orbit, yet we have seen that the duration  of the
           summer or winter does vary as the  ecccenticity.  Supposing, there-
          fore, that we have the  longest  winter  in  the  northern  hemisphere,
           we shall have to distribute 229  heat-units over 166 days of a short
          summer,  and 136 heat-units over  199 days of a long winter of the
          same  period.  In  other  words,  the  difference  between  the  daily
          average  heat  in  summer  and  winter  will,  in  such  a  case,  be  the
          greatest,  producing  shorter  but warmer  summers  and  longer  and
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