k t !• 
C 324 ] 
If a like computation be made from the 16th obfervation, 1 , 
it will be mund ' V 5 26 a i 
By comparing feme other obfervations with thefe, I con'- g 
dude, the time of the leaft diftance of the centers was / ^ ^ 
// 
Then as radius to tangent of the angle 1 o’ ~ 
of the ecliptic, with path of Venus j ^ ^7 
So is the leaft diftance of the centers 610 
9.i73>57* 
2,78^3298 
To the diftance of Venus’s place, when 
nearell the Sun’s center, from her . 
place at the time of ecliptic con- 
junftion 
90,88 1,9584869 
h ^ 
It 
Which reduced to time (to be fubtrafled) viz. o 22 41 
From time of the leaft diltance of the centers 5 26 20 
Leaves for the time of ecliptic conjunction 
5 3 39 
As radius to fecant of 
So is 
o t n 
8 28 27 
610 
10,0047676 
2,7853298 
To the geocentric latitude of Venus at | 2,7900974 
the time of ecliptic conjunction J . 
From the logarithm of which fubtraCl the difference of the "j 
logarithms of the diftance of Venus from the Earth and >0,4002370 
from the Sun • J 
Remains the logarithm of the 1 , ^ 
- j ^ ^ ^’39 
heliocentric latitude 
2,3898604 
O t 
As tangent of inclination of Venus’s orbit 3 23 20 
To ra^us; fo is tangent of Venus’s helio- \ 
centric latitude J° ^ . S >39 
To the fine of her difiance from nede in 1 
the ecliptic | ^ V 4 
8,7724442 
7,0754375 
8,302993.3 
The 
