( *4 8 )

wherc that former from Scient cxactly anders to the Rccent; and that fromAJ nrcab ’tis true, differs in a very fcw Seconds, but that difparity is of nomomen'-, linee it only procecded from thencc, that this New Star is not yet16 dillinctly to be lecn as at that time, when it was of the Third Magnitudc.Jt is therefore - ccrtain, that it is the lelf-lame Star, which Kspler did sirst secAnn. 1601. and-continued tiil Anu, 1661. He that will observe this Star,nuist take care lest he mistake the Three more Southern ones of the Sixth

Magnitudc - the Highest of which is distant from Sebent Pegas, 3 6°. 25^. 45

... ‘ ‘ 4 - 30"

and the Lowest 38^in Pcclon Cygni quae aliquam-lereno quali Reviviscere vide-

( etiam Luna lplendentc^) appa-

I.. L5. f .2 089.

. 11 , 134 -

the Aliddlcmost from tlic time 37“. 25. xo'

1 34 * s- 3 55 - Ann. 1 56 y, Novetnb. 2 3 . Stella illa novadiu ab Anu. 1 66z. plane dilituit, Coelobatur.

Ann. t666. Septemb. x\. Nudis Oculisruit. Sept, 2.4. Minor erat illis tribus praecedentibus,in Collo & vix (T Magn.videbatur.

Ann. 1670. Aug. 26. 'Sensim Crefcerc videtur quanquam necdum Majorest Stellis 6 Magre Sept. 3. Adhuc Creseere videbatur; 8. Paulo adhuc Crcl-f. 855. cere deprehendimus ; Sc Ollob. 13. Satis clare apparuerit.

Ann. 1671. April. 29. Vix major adhuc apparuit quam Anno Praeterito.-,si quidem Stellis 6 Magn. xquabatur.

Ann. 1671. Jun. 2 6. Major fere videbatur.

Ann. 1672. Mnrt. 29. Adhuc Crelcere videbatur.

Ann. 167y. Jul. 22. Apparuit instar 6 Magn.n, 134. f. 854. Ann. 1677. Nondum ad priorem Magnitudinem (Tertii videlicet Ho-noris) atque Claritatem & Splendorem (qua Magnitudine Ann. 165-7, 1658,& 1659. apparuit) pervenit: siquidem non nili instar 6 Magn. adhucfulget.

Ann. 1681. Aug. I 8. Nova in -Collo Cygni, Nudis Oculis ob ejus tenui-tatem parvitatemque haud quidem conlpecfa, sed Telefcopio tamen depre-hen'a est.

4. i.Don Anthcltnc, a Carthufian at Dyon, on the 20th of June,Ann.-t 6 jo.dilcovercd a Star of the Third Magnitudc beneath the Hcnd of Cygnus, si-tuated in the Secfion of the two streight Lines, one of which goeth fromLyrn to the nearest of the Quadrangle in the Dolphin, and the other fromthe F.nglc to the Star, which is on the top of the Vppcr Pf wg of Cygnus.He lent the News of this Diseovery to M. JL’ Abbe Mariotte, one of the l{oyalAcndemy , who communicated it to the rest. They all agree, ’tis a Kctv Star j

though M. B .opposed it at first, afiirming it to be in Bayeruss Ta-

blcs: but they prove that Star in Bnycrus to be another; giving for diltin-.guifliment thele Mfcaliires.

Tb . Col . n, 5.,J>. I Ü2.

The AVm Sfj/b'Capitc-Cygni-,ji. 65. f

M. 7 i- f

2092,

2198.

The Bright Star ad 'Bofirum

But this .\em Star’s Ascensit J{ccia, is

lt’-s Ascensio Becln.Declinatio Borealis.

Declinatio Borealis.

0

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