36.3 UEPORT— 1872. 



will be the hour-angles of the ideal stars. These have been calculated by 

 successive additions for each integral mean solar hour of the year, and 

 subtraction of 360 every time a number exceeding 360 has been reached ; 

 and the results have been tabulated. Preceding each hour-angle, the num- 

 ber which, multiplied by 15, most nearly agrees with it has been written. 

 The following is a specimen page for one day of the Table thus formed : — 



