(mo) 
/. d. m. fee. 
The Moon from the Horofcope in the Ecliptick 47 34 
In a great Circle 47 3^ 
Her Azimuth from the Horofcope 45 53 
The Altitude of her Center 1423 
Her Parallaftical Angle 78 17 
C Altitude 51 21 
Her Parallax in < Longitude 10 25 
<! Latitude 50 17 
Hence her vifible place m 29 J 4 48 
With vifible North-Latitude i 8 59 
Therefore ftie is in Antecedence of the Star 1 5 2 5 
With lefs North Latitude 1 6 1 
Now the Moons Semi-diameter being only 14«;. 17 fee, it 
appears , that the Star is more to theNorth, than the Moons 
Limb 5 hyim 44 fee, and the Moons Latitude dccreafing toge- 
ther with the Altitude of the pjddegree^caufeth the Affarent 
Motion to be vijfible in aline bending down from the Star 5 fo 
that near the vifible ConjunAion the Star may ftand about 3 min* 
to the North from the Moons Limb. Though this be not like 
roprovcanOccukacion , yet let me deiirethofe , who hare fit 
GlafFes andlnftruments to obferve this Trartp, and how far 
the Star may ftand from the Liml> of the Moon at the time of the 
vifible Conjun(ftion , that we may be the better enabled to de- 
fine, hth ho^ the Motion of the Moori's Latitudes, which 
fliall need its limations , is to be reformed 5 4;^/ whether that JE- 
qmtion of the Nodes , allow'd by the Car^lim Author andfome 
other Moderns, be firm and valid, 
F. The laft Occultation happens on May 23 5 when 1 2 7 
F, M, by the Efhemerides the Moon will be in Conjuncftion with 
Antares. To define the Beginning and End of it, I have fnp- 
puted the Moon's true and Vifible places to 1 2 h. 2 8 mm. 42 fee^ 
and 1 3 k 43 ^o'fee, P. M, at Dedj 5 by the Carfilif^e T abUsy 
ami ifind^ - 
The 
