C 1 
vations, that the Motion of this Cornet in its own 
Orbit was c DireEl> and that it was in its Perihelion, 
January 19. 8 H. 20 Min. Temp. <^yEquat. Lond. 
That the Inclination of the Plane of the Trajectory to 
theEcliptick was 1 8 Deg. 20 Min. 45* Sec. The Place of 
the Descending Node 16 Deg. 22 Min. The Place 
of the Perihelion & 2 f Deg. 55 Min. The Diftance 
of the Perihelion from the Descending Node 80 Deg. 
27 Min. The Logarithm of the Perihelion PDiJlance 
from the Sun 9.347960. The Logarithm of the Di- 
urnalMotion 0.938188. 
From thefe Elements (by the Help of Dr. Halley s 
general Table for Comets, to which they are adapted) 
I computed the Places in the following Table 5 which 
alfo contains the Longitudes and Latitudes of the Co- 
met, calculated from the obferved Right Afcenfions 
and Declinations above-mentioned, together with the 
Differences between the obferved and computed 
Places* 
Oxon* 
