(iioj) 
d, fn. fec^ 
Her vlfible Motion from 7 28 to 8 1 8 1». is o 22 52 
The diference of the Moons vifiblc Latitudes o 2 45 
TheAngleohheMoonsvifible way with the Eclip. 6 51 27 
Her vifible Latitude at the apparent Conjunction i 35 12 
The Angle of Immerfion beneath a ftraight^ 
line drawn through her Center parallel coS**— • 5^33 5 
the Ecliptic 3 
Motion from the /inmerfion tJO the vifib. Conjund. 0 9 i 
The Aogle of Ernerfion beneath the parallel 3 7 42 J 
The viliD* Motion from the o ^,to the Egrefs appar, o 11 30 
Apparent Mot. fr©m '^h. 28 tothe Immerfion 0 03^ 
Apparent Mot. from 8 1 8 to the Stars Egrefs o i 5 5 
The time from 7 28 to the Sub-ingrefs o 2 9 
Thetimefrom 8 18 to the Stars EmerC o 4 22 
Therefore the Sub-ingrefs 7 2^ 6, 
Emerfio« 8 13 38, 
The Stars ii/^r^ under the Moon o 44. 32, 
The Stars Latitude from a line 1 r Immerfion 11 17 
drawn over the Moons Cen- > in the \ 
ter parallel to the Ecliptick J ^Egrffs 8 50 
Over what Spots of the Moon, the feemingwayof the Star 
would pafs 5 /do not herefhew, becaufe I dare not rely on our 
Selenographical Tables. / proceed therefore to the next, 
///. Marsh 3. in the morning , the Moon pafTeth over Ant^- 
res^ or the S€»rf ions heart ^ whofe Longitude to the Caroline 
Author is then Scorpio % deg, 7 m. 20 fee, and Latitude South 4, 
27. The Ecliptical Conjunftion by the Bfhemerides was March 
2. i6h,^^m. F.M. Wherefore 5 for the better inveftigating 
the times of the beginning and end of this Occultation, /have 
calculated the true and vifible places of theMoon to i6k ^gm,, 
52 fee. and to 17 A. 49 m. ^ifec^ M, by the faid Tables to 
the Meridian and Latitude otDer^j^ as follows § 
Ooooo 
