GEORGIUM S/DUS. 



tion Jecreafes, fubtraAed fi-<Dm4".7 leaves4".i, the equation 

 required. By proceeding thus to argument VIII. we get 

 all ihe equations, and by taking the difference of the poli- 

 tive and negative parts, we get 3''2l'45".5 fur the value 

 of the firft eight equations ; which applied to 4' 10" 6' 1 1 ".4 

 gives 4 6 47' 25 '.9 the longitude of the Georgian in his 

 orbit. From this longitude fubtraft 2' 12 48*19' the 

 longitude of the node, and we get i' 23' 5:6' 7 ", which is 



argument IX.; with which enter Table XVII. and take out 

 thereduftion, which is— 8".9,andthisappliedt04 6 44'25''.9 

 gives 4 6 44' 17', the heliocentric longitude of the Geor- 

 giun on the ecliptic from the mean equinox. Alfo with ar- 

 gument IX. enter Table XVI. andtakeoutthe latitude. Now 

 for I' 23 ' the latitude is 36' 57'', and it increafes 28".8 for 60'; 

 hence 60' : S^"-7 '• '• 28'. 8 : 26". 9, which added to 36 ^7" 

 gives 37' 2 3 ".9, the heliocentric latitude of the Georgian. 



Table I. 

 Epochs of the mean Longitude of the Planet, with the Arguments of the Equations. 



