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to Lecture XL

^ar an a S°lft* ces -> b y considering the several(y a the y pass’d through among the otherJ 0jf ^ Rations, as follows, according to Eu~

a' tbe ® aG k ^ r * es 1S a Star of thegnitudc, marked 7 by Bayer ; i n the* <* the Year 1689, its Longitude was

38 45^; and the Equinoctial Colurethrough, according to Eudoxus , cuts^ cb ptic in 8 6° 58' 57".

In the Head of Cetus are two Stars

of

^ e ' 4th Magnitude, called v and I byfyjj * Eudoxush Colure passing in thek ^ e between them, cuts the Ecliptic in^ 38' ^1^, a t the End of the Year 1689.^ the extreme Flexure of Eridanusw as formerly a Star of the 4th Mag-Qet e (of late it is referred to the Breast of\ Q '• It is the only Star in Eridanus ,which this Colure can pass ; its

Vis

V e was at the End of the Year 1689^ ^2 io", and the Colure of the Equi-

ps

Pass12

r

ssg through it cuts the Ecliptic in

, So / 4 °~

!>a^' the Head of Perseus , rightly de-

a Star of the 4th Magnitude,

If T ^f Bayer; its Longitude was y 23®

at the End of the Year 1689; and

the