O] 
Eqmno&ial and Solflitial Colures, and the Scries of 
Obfervations of it is fomewhat more complete, than 
that of t Terfei ; I fhall infert one at lcaft, for each 
Year wherein it has been obferved 5 whereby it may 
appear, that the Hypothefis folvcs the Thcenomena 
of Stars in this Situation, as exactly as in others : 
for if a mean be taken of the Numbers in the lah 
Column of the following Table, which exprefles the 
mean Dihance of the Star South of 41 ,J . y'. on 
March 27th 1727, it will agree within two Seconds, 
with every one of 80 Obfervations, that have been 
made of this Star. 
« Terfei 
South ot 
0 / 
4T. , 5 
Precet- 
fion. 
Aberra- 
ration. 
Nutation 
Mean 
D;ft. 
South. 
1727 December 29 
1728 April 7 
July 5 
December 13 
/1 
79 4 
* 7.5 
94.6 
C" 7 
/ 1 
T 10 5 
14.3 
17-7 
238 
// 
+ n -4 
— 0.8 
— 1 1.4 
4. io.'6 
// 
+ 7 9 
8.2 
8.5 
8.8 
// 
109.2 
109 2 
lo 9 4 
108.9 
1729 December 3 
1731 January 3 
t732jinuary 8 
1 73+ July 11 
5 V 4 
38 6 
26 8 
S. 213 
37.2 
52.3 
66 . 2 
101 0 
97 
11. 4 
+ n -4 
__ 11. 4 
89 
78 
+ 59 
— 11 
109 2 
£10.1 
t IO.3 
IO9.8 
1738 December 24 
1 740 January 21 
174"' February 27 
N. 50.3 
718 
182.5 
162.6 
x 77-4 
2 75-4 
-f" ii- 2 j 90 
10 9 — 82 
6 6 |q_ g 5 
108.5 
to8 3 
[08.0 
Having already given Examples of Stars, lying near 
both the Solfticcs and the Vernal Equinox 5 1 (hall 
now add the Obfervations ot one , that is not far 
from the Autumnal Equinox, viz. » Ur fa Major is , 
the brighteft Star in that Part of the Heavens, which 
approaches the Zenith of JVanfted within a Degree 5 
and 
