( ) , , 
on the fide of the Comet a ftar fufEcieotly clear^whicli was mt 
further diftant from hiaij than a iitde more than the diaoietec 
of rhtfCometj and chat was Vt the fatos height of the Horizon - 
which may fcrve to determine the paraHax^iiiht fame ubfcrva. 
iron be, made eKwhere* , ' 
in the evenings the Comet- was equahy diftant 
from the inferior ftar of the Northrea E^r ofTdwus^ and from^ 
the fuperior of the root of the Northren horn. He was aUo as 
krdiftaot from this latter ftar, as tWsftar is froai that of the 
fronuThis place^beiog carried over to the Map of the fi-st ftar?,, 
feil on S.deVrees and goV olGemm, in the Northren lacir.of i. 
degree and }6'. As we were preparing to obierve wiihthe great 
Teicfcope^the Heaven was clouded over. 
JpniiB.^.md 10, we could make ooobfervation atall^ be- 
caofe of theconftant dark weather. 
Sijj^mr Caffnii's repawns on thefoYegoing ohfervations. 
!i the places of the Comet^that we have obfervcd cilfnow, 
_ _ fail into a Une little differing from an Arch of a gre^t Cir- 
de^which cuts the Ecliptique in the 10/^. deg45'.ofG(?w?W5and 
which confeqoently hath its greateft latitude in the ic/Me.- 
greeand45,\ ofP^y^^^ 5 which latitude is between 39* and 401 
deg Nord^ward. The fame Circle cuts the Equator loi. de- 
grees of the Vernal iSedion Eaft^ward, and its greateft decJi* 
nation from the £f?M^Gr Nord."Ward is of 3§^ degTees, 
Whence it follows, that the Comet at the time of his greateft 
Dedination^wherein it may have ftay'd a confiderablc time,: 
hath toiich'd the horizon of thofe that are in tiie latitude of ; r-- 
degreesithe parallel of whom pafietb through the lower part of 
Eli^afd^md through^aldnd^WeflphaIia,Saxony^ Poland &cc:And 
that he hath reosain'd at that time all night and all day above 
the horizonof the moft Northern people 5 as are thofe of the 
upper part of Engiancl,Hollcind,Pomerama^ &c. But that he hath 
f xkd through theZenith ofthe lower part ofSpam^znd through 
Sardima^Calakia^Chio without having beeo-per- 
ccived in rhofe places^ becaufe he there pafs'd in the day- time. 
••5incc%e cosldnqt fee this' Comet but about the end of 
Marm^ wc have made ofeof our method explained in the-The- 
my of the Comet of the ye^r 1665 ^ to, find the places where-' 
iiboifr thir Comt!t 'ftath'bcen daring^the raoneth oiMarch^ ifl 
$lie tiy:p^:hvS:S.0iUac equal te^riline^t®> 
■ , , lepr^^' 
