C 3 
in. If Ngtn. II. thus equated exceed Subftrad 
^%,4 therefroni ; and if the remainder or Nurn. IL be 
lefs'tfaan iijjWith the (aid remainder or Namber j or if 
greater than 113, with the complement thereof to ix 5',4. 
feek in Table pag, %^6. the fecond ^Equation, which be- 
ing added tro the Time before found, gives the true Time 
of the middle of the Echpfe. 
IV. With Num. T. in Tah. pag. 247, feek the half 
Continuance of the Total Eclipfe, which is to be added 
: for the £frterJton when the ^equated Num. II. is lefs than 
113, or if more than xi j^, it be left than 338. But 
if it exceed 113 or 338, then is thQ Semimra to be 
M>&.iMl^td for the Immerfi^^^ 
V. Laftly, with the Sun's true Place take out the 
I ^Equation of Natural Days ( in Tak pag 248. ) which 
! ^Ided or fiibftrafted according to the Title, gives the 
' lime of t|ie Immerjion or Emerfon fought. 
Now how ftw Figur^es ferve for this Computation , 
will bcft appear by an Example or two» 
. " Annoi 6y'j. Septemher 17^^- 8^- 9'. 40'^ ^tGremwkh^ 
I obferved the iitUt Satellite to begin to 
^fitir^ ^ that is 8^- 9'. %d'. London, 
riJiw^fcifti^^fi 
iEquat. r. 
4 
__4 
36' 
12 
17 7 
18 
26 
48 
II 
.^quat. 2. 
EquU Time 
^Equation 
Appar. T. 
Obfer. 
+ 
I 
37 
39 
o 
Num. I. 
2028 
2i7y 
2448 
273 
Num. A. " ' 
248jO 
2,3 4* 
250,3 
16 
IS 
11)26,2(2,3+. 
© in ^ 5*^00 
24,9 
17 
Erfor^ 
10 
9 
41 
20 
21 
Again^ 
