< w ). 
15:74, after fixteen Months, to be no longer vifible; and 
at this Day no Signs of it remain. The Place thereof 
in the Sphere of Fixt-Stars, by the accurate Obfervati- 
ons of the fame Tycho, was os. 9 0 . 17'. d i ma ^ r ,s , with 
55°. 45'. North Latitude. 
Such another Srar was feen and obferved by the Scho- 
Jars of Kepler, to begin to appear on Sept. 30°. ft. vet. anno 
1604, which was not to be feen the Day before; but it 
broke out at once with a Luftre furpafling that of Jupiter; 
and like the former it died away gradually, and in much 
about the fame time difappear’d totally, there remaining 
noFootfteps thereof in January i6o|. This was near the 
Ecliptick, following the Right- Leg of Serpentarius ; and 
by the Obfervations of Kepler and others, was in 7 s . io°. 
oo'a i m3 4c.V, with North Latitude 1 56'. Thefetwo 
feem to be of adiftind Species from the reft, and nothing 
like then} has appear’d fince; 
But between them, viz,, in the Year 1596, we have 
the firft Account of the wonderful Star in Cello Celt , feen 
by David Fabriciits on the third of Augufl, ft. vet. as 
bright as a Star of the third Magnitude, which has been 
fince found to appear and difappear periodically : its Pe- 
riod being precifely enough 7 Revolutions in Six Years, 
tho’ it return not always with the fame Luftre. Nor is 
it ever totally extinguilh’d, but may at all times be feen 
with a Six-Foot Tube. This was fingular in its Kind, 
till that in Cello Cygni was difeovered. It precedes the 
firft Star of Aries i°. 40', with i?°. 57' South Latitude. 
Another New Star was firft obferved by Will, fanfonius 
in the Year 1600, in Pettore or rather in e duff i one Colli 
Cygni , which exceeded not the third Magnitude. This 
having continued fome Years, became at length fofmall 
as to be thought by fome to difappear entirely : but in 
the Years 1657, 58 and 59, it again arofe to the third 
Magnitude, tho’foon after it decay’d by degrees to the 
I i i z fifth 
