Page 256 - Lokmanya Tilak Samagra (khand 2)
P. 256

THE  ARCTIC  REGIONS                43

            horizon  of  the  observer  will be · H' H, atid  the  stars  will :  ·now
           appear to move in circles  inclined  to his  horizon, as shown in the
                                            figure  by the  black lines AA',
                                            BH'  and  CC'.  Some  of the
                                            stars,  viz.,  those  that  are
                                            situated  in  the  part  of  the
                                            celestial dome represented by
                                            H'PB,  will  be visible  throu-
                                         0  ghout  the  night,  as  their
           H'f:::::::>"~-r'--~~...,.~..:::::::::_~H  circles  of revolution  will  be
                                            above the horizon H' C' D H.
                                                                  1
                                            But  all  the  stars,  whose
                                            Polar  distance  is  greater
                                            than  PB  or  PH',    will
                                            in  their  daily  revolution,
                                            be  partly  above  and  partly
           below  the  horizon.  For  instance,  the  stars  at  C  and  D  will
           describe  circle  ,  some  portion  of  which  will  be  below  the
           horizon  H' H.  In  other  words,  the  appearance  of  the  vi  ible
           celestial  hemi phere  to  a  person  whose  zenith  i  at Z  will  be
           different  from  the  appearance  pre ented  by  the  heavens  to  an
           ob  erver at the  orth Pole.  The  tars will  not  now  revolve  in
           horizontal  planes,  but  obliquely.  A  great  number  of them would
           be  circumpolar  and  visible  during  the  whole  night,  but  the
           remaining  will  rise  and  set  as  with  us  in  the  tropics,  moving in
           oblique circles.  When Z  i  very  near  P, only  a  few  star  will  rise
           and set in  this  way  and the  difference  will  not be  a  marked  one;
           but as Z  i3 removed further south, the change  will  become  more
           and  more  apparent.
               Similar  modification  will  be  introduced  in  the  duration  of
           day and night, when the ob erver's position is  hifted  to  the south
           of the terrestrial  North Pole.  This will  be clear  by  a  reference  to
           the figure  on the next page.  Let P  be  the cele  tial  orth Pole and
           Q' Q the celestial equator. Then  ince the sun moves in  the ecliptic
           E' E, which is  inclined at an angle of about  23i  0   (  23°  28')  to  the
           equator, the circles T E and E'T will corre pond with the terrestrial
                              1
           circles  of latitude  called  the  Tropics  and  the  circle  AC with  the
           Arctic  Circle  on  the  terrestrial  globe.  Now  as  the  sun  moves
           in  the  ecliptic  E' E,  in his  annual  cour e  he  will  always  be  twice
           over-head for an.observer stationed at a place within the terrestrial
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