of the Places of the Stars. 



27 



ning of 1815, which will be sufficiently accurate, even if we 

 omit his ten thousandths of seconds. 



Correction of the right ascension of « Ursse Minoris in time, 



= iV (*' ~ *)• 



+ 20' ,368 sin. (S3 + 256=. 40 ',9) 



+ ,194 COS. 2 g, 



+ 1,327 sin. (2 © + 254° .46',9) 



+ ,201 sin. (2 C +253°. 44') 



+ ,011 sin. (2 gj +329°. 24') 



+ 42,519 sin. ( Q + 254o.50' .7) 



+ ,071 sin. (2 O + 332°. 0') 



+ ,057 sin. (o + S3 + 332°. 23') 



4- ,010 sin. (©_$?+ 343°. 54') 



+ ,712 COS. <p COS. (f* - 13°. 57'), 



For the declination, y — ^. 

 + 6",837 sin. (^ + 161°. 32',5) 

 — ,021 COS. 2 S2 



in. (2 O + 163°. 48'.) 



in. (2 C + 164°. 51') 



in. (2 Si + 232°. 28') 



in. (O + 167°. 48',8) 



in. (2 O + 227°. 30') 



in. (O + Q + 2460. 30) 



in. (O — R + 264°. 50') 

 sin. (/* — 130. 57'). 



The angle (p is the latitude, and /* the sidereal time ex- 

 pressed in degrees. The laborious author promises new tables 

 of the pole star, calculated upon these principles, which will 

 be published in the fourth part of his astronomical observa- 

 tions. S. B. L. 



