Page 39 - Lokmanya Tilak Samagra (khand 2)
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26             SAMAGRA  TILAK - 2  •  THE  ORION

         The  Vedic  observations  could not  again  be  such  as  need  any
         minute or detailed arithmetical operations.  I shall therefore adopt
         for  the  present  the  simplest  possible  method  of calculation,-a
         method which may be easily understood and followed by any one;
         who  can  watch  and  observe  the  stars  after  the  manner  of the
         ancient priest. We shall assume  that the  zodiac  was  divided  into
         27 parts, not by compass but by means of the leading stars, which
         Prof.  Max MUller rightly calls the milestones  of the heavens.  The
         Vedic priest, who ascertained the motion of the sun by  observing
         with  his unaided eye the neares~ visible star, • cannot be  supposed
         to  have  followed  a  different  method  in  making  other  celestial
         observations; and if so, we  cannot assume that he was capable of
         recognizing  and  using  for  the  purposes  of observation  any  arti-
         ficial  divisions  of the  ecliptic  pn  a  mathematical  principle,  such
         as those which would result from the division of 360° of the  zodiac
         into  27  equal parts,  each part thus extending over·  130  20'  of  the
         ecliptic.  Of course,  such an artificial  method might  be  easily  foll-
         owed j.n later days, when the means  of observation increased and
         the  sclcnce  of arithmetic  was  developed.  But  in  the  earliest  days
         of civilization,  it  is  more natural  to suppose  that  the  motions  of
         the  sun  and  the  moon  were  determined  by  observing  which  of
         the known fixed  stars was  nearest  to  them.  When  we,  therefore,
         find it stated in the Vedic works that the sun was  in the  K~ittikas,
         it is  more probable that the fixed  asterJsm,  and  not the beginning
         of the artificial  portion of the  zodiac,  was  intended. I  admit that
         the  accuracy  of such  observations  cannot  be  relied  upon  within
         two  or three degrees,  if not more.  But we  must  take  the  facts  as
         they  are  especially  when  it  is  impossible  to  get  anything  more
         accurate  from  the  ancient  observers  of the  heavens. t  It will,  I
         trust,  however,  be found  that this  inevitable  want  of accuracy  in
         the old observations does not affect our conclusions to such an ex-

            •  Taitt.  Br.  1.  5·  2.  J,  pre'\·iously  quoted.  The  passage  is  very
         importan'tn-.4  describes  the  method of  making  celestial  obserntions
         rn  old  times.
            t  Similar observations have been recorded by  Greek  poets.-Homer
         mentions  'the  turns  of  the  sun, '  and  Hesiod  • the  -rising  and  the
        setting o( the Pleiades at the beginnings of day and night.'  The  obser-
         vations in the Vedic works may  be supposed  to  have  been  made  i R  a
         similar way.
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