1& poſitiones fixarum inter ſe & poſitiones Cometæ ad fixas de
terminavimus. Deſignet Aſtellam in ſiniſtro calcaneo Perſei
(Bayero o) Bſtellam ſequentem in ſiniſtro pede (Bayeroζ) &
C, D, E, F, G, H, I, K, L, M, N, Oſtellas alias minores in eo
dem pede. Sintque P, Q, R, S, Tloca Cometæ in obſervati
onibus ſupra deſcriptis: & exiſtente diſtantia ABpartium (80 7/12),
erat ACpartium 52 1/4, BC58 5/6, AD(57 5/12), BD(82 6/11), CD23 2/3,
AE29 4/7, CE57 1/2, DE(49 11/12), AI(27 7/12), BI52 1/6, CI(36 7/12),
233[Figure 233]
DI(53 5/11), AK38 2/3, BK43, CK31 5/9, FK29, FB23, FC36 1/4,
AH18 6/7, DH50 7/8, BN(46 5/12), CN31 1/3, BL(45 5/12), NL31 5/7.
HOerat ad HIut 7 ad 6 & producta tranſibat inter ſtellas
D & E,ſic ut diſtantia ſtellæ Dab hac recta eſſet 1/6CD. LM
erat ad LBut 2 ad 9 & producta tranſibat per ſtellam H.His
interminabantur poſitiones fixarum inter ſe.
terminavimus. Deſignet Aſtellam in ſiniſtro calcaneo Perſei
(Bayero o) Bſtellam ſequentem in ſiniſtro pede (Bayeroζ) &
C, D, E, F, G, H, I, K, L, M, N, Oſtellas alias minores in eo
dem pede. Sintque P, Q, R, S, Tloca Cometæ in obſervati
onibus ſupra deſcriptis: & exiſtente diſtantia ABpartium (80 7/12),
erat ACpartium 52 1/4, BC58 5/6, AD(57 5/12), BD(82 6/11), CD23 2/3,
AE29 4/7, CE57 1/2, DE(49 11/12), AI(27 7/12), BI52 1/6, CI(36 7/12),
233[Figure 233]DI(53 5/11), AK38 2/3, BK43, CK31 5/9, FK29, FB23, FC36 1/4,
AH18 6/7, DH50 7/8, BN(46 5/12), CN31 1/3, BL(45 5/12), NL31 5/7.
HOerat ad HIut 7 ad 6 & producta tranſibat inter ſtellas
D & E,ſic ut diſtantia ſtellæ Dab hac recta eſſet 1/6CD. LM
erat ad LBut 2 ad 9 & producta tranſibat per ſtellam H.His
interminabantur poſitiones fixarum inter ſe.
Die Veneris Feb.25. St. vet. Hor. 8 1/2 P. M. Cometæ in pex
iſtentis diſtantia a ſtella Eerat minor quam (3/13) AE,major quam
3/5 AE,adeoque æqualis (3/14)AEproxime; & angulus ApEnon
nihil obtuſus erat, ſed fere rectus. Nempe ſi demitteretur ad
pEperpendiculum ab A,diſtantiæ Cometæ a perpendiculo illo
erat 1/5pE.
iſtentis diſtantia a ſtella Eerat minor quam (3/13) AE,major quam
3/5 AE,adeoque æqualis (3/14)AEproxime; & angulus ApEnon
nihil obtuſus erat, ſed fere rectus. Nempe ſi demitteretur ad
pEperpendiculum ab A,diſtantiæ Cometæ a perpendiculo illo
erat 1/5pE.