/laS A Talk njihe Rediiclmi of the Ecliptic, &c. [Tab. IV.] 



TABLE continTU'.l. 



Enter tlie Table with tlie Lnngiiutle of tbe Ecliptic as tlie Argument, nml 

 take out the correspoudiug i eduction, applying the correction (or the variation 

 of tiie Obrniuitv according as it is more or less than 23 ' 27' 57". This Equa- 

 tion apjjiicd according to its sign to the Longitude of the point of the 

 Ecliptic gives the Sun's Right Ascension as rc(iuircd. 



LXXXII. Fari' 



