10 Persei
Appearance
Coordinates:
02h 25m 16s, +56° 36′ 35″

Observation data J2000
| |
---|---|
Constellation | Perseus |
Right ascension | 02h 25m 16.02834s[1] |
Declination | +56° 36′ 35.3544″[1] |
Apparent magnitude (V) | 6.26[2] |
Characteristics | |
Evolutionary stage | Blue supergiant |
Spectral type | B2Ia[3] |
U−B color index | −0.61[2] |
B−V color index | +0.30[2] |
Variable type | α Cyg[4] |
Absolute magnitude (MV) | −6.70[6] |
Details Myr | |
SAO 23304, GC 2885 | |
Database references | |
SIMBAD | data |

10 Persei is a blue supergiant star in the constellation Perseus. Its apparent magnitude is 6.26 although it is slightly variable.
10 Persei is located around 3,333 parsecs (10,870 ly) distant in the Perseus OB1 stellar association. It lies close to the Double Cluster and is considered a cluster member.[7]

In 1999, 10 Persei was given the
variable star designation V554 Persei, after being identified as varying in Hipparcos photometry.[9] Its brightness varies by less than a tenth of a magnitude with no clear period.[4]
References
- ^ S2CID 244398875. Gaia DR3 record for this source at VizieR.
- ^ Bibcode:2002yCat.2237....0D.
- .
- ^ Bibcode:2009yCat....102025S.
- ^ ISSN 0004-6361
- S2CID 1552752.
- S2CID 14252530.
- ^ "Hipparcos Tools Interactive Data Access". Hipparcos. ESA. Retrieved 8 December 2021.
- Bibcode:1999IBVS.4659....1K.
Further reading
- Crowther, P. A.; Lennon, D. J.; Walborn, N. R. (2006). "Physical parameters and wind properties of galactic early B supergiants". Astronomy and Astrophysics. 446 (1): 279–293. S2CID 18815761.
- McErlean, N. D.; Lennon, D. J.; Dufton, P. L. (1999). "Galactic B-supergiants: A non-LTE model atmosphere analysis to estimate atmospheric parameters and chemical compositions". Astronomy and Astrophysics. 349: 553. Bibcode:1999A&A...349..553M.