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10 Persei

Coordinates:Sky map02h 25m 16s, +56° 36′ 35″
From Wikipedia, the free encyclopedia
Blue supergiant star in the constellation Perseus
10 Persei
Location of 10 Per (circled)
Observation data
EpochJ2000      EquinoxJ2000
ConstellationPerseus
Right ascension02h 25m 16.02834s[1]
Declination+56° 36′ 35.3544″[1]
Apparent magnitude (V)6.26[2]
Characteristics
Evolutionary stageBlue supergiant
Spectral typeB2Ia[3]
U−Bcolor index−0.61[2]
B−Vcolor index+0.30[2]
Variable typeα Cyg[4]
Astrometry
Radial velocity (Rv)−39.87±1.93[1] km/s
Proper motion (μ)RA: −0.508mas/yr[1]
Dec.: −1.182mas/yr[1]
Parallax (π)0.4424±0.0263 mas[1]
Distance7000±815 ly
(2,150±250 pc)[5]
Absolute magnitude (MV)−6.70[6]
Details[5]
Mass23.6±1.9 M
Radius49±6 R
Luminosity257,000 L
Surface gravity (log g)2.45±0.07 cgs
Temperature18,600±300 K
Rotational velocity (v sin i)48±6 km/s
Age7.76 Myr
Other designations
V554 Persei,HR 696,HD 14818,BD+55°612,HIP 11279,SAO 23304,GC 2885
Database references
SIMBADdata
10 Per is the bright star below and right of the Double Cluster

10 Persei is ablue supergiant star in theconstellationPerseus. Itsapparent magnitude is 6.26 although it is slightly variable.

10 Persei is located around 3,333 parsecs (10,870 ly) distant in thePerseus OB1stellar association. It lies close to theDouble Cluster and is considered a cluster member.[7]

Alight curve for V554 Persei, plotted fromHipparcos data[8]

In 1999, 10 Persei was given thevariable star designation V554 Persei, after being identified as varying inHipparcos photometry.[9] Its brightness varies by less than a tenth of a magnitude with no clear period.[4]

References

[edit]
  1. ^abcdeVallenari, A.; et al. (Gaia collaboration) (2023)."Gaia Data Release 3. Summary of the content and survey properties".Astronomy and Astrophysics.674: A1.arXiv:2208.00211.Bibcode:2023A&A...674A...1G.doi:10.1051/0004-6361/202243940.S2CID 244398875. Gaia DR3 record for this source atVizieR.
  2. ^abcDucati, J. R. (2002). "VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system".CDS/ADC Collection of Electronic Catalogues.2237.Bibcode:2002yCat.2237....0D.
  3. ^Kraus, M.; Borges Fernandes, M.; Kubát, J. (2009)."Parameters of galactic early B supergiants. The influence of the wind on the interstellar extinction determination".Astronomy and Astrophysics.499 (1): 291.Bibcode:2009A&A...499..291K.doi:10.1051/0004-6361/200810319.
  4. ^abSamus, N. N.; Durlevich, O. V.; et al. (2009). "VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)".VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S.1.Bibcode:2009yCat....102025S.
  5. ^abWeßmayer, D.; Przybilla, N.; Butler, K. (2022-12-01), "Quantitative spectroscopy of B-type supergiants",Astronomy & Astrophysics,668: A92,arXiv:2208.02692,Bibcode:2022A&A...668A..92W,doi:10.1051/0004-6361/202243973,ISSN 0004-6361
  6. ^Searle, S. C.; Prinja, R. K.; Massa, D.; Ryans, R. (2008). "Quantitative studies of the optical and UV spectra of Galactic early B supergiants. I. Fundamental parameters".Astronomy and Astrophysics.481 (3): 777.arXiv:0801.4289.Bibcode:2008A&A...481..777S.doi:10.1051/0004-6361:20077125.S2CID 1552752.
  7. ^Lee, Hsu-Tai; Lim, Jeremy (2008). "On the Formation of Perseus OB1 at High Galactic Latitudes".The Astrophysical Journal.679 (2):1352–1363.arXiv:0804.4520.Bibcode:2008ApJ...679.1352L.doi:10.1086/587801.S2CID 14252530.
  8. ^"Hipparcos Tools Interactive Data Access".Hipparcos. ESA. Retrieved8 December 2021.
  9. ^Kazarovets, E. V.; Samus, N. N.; Durlevich, O. V.; Frolov, M. S.; Antipin, S. V.; Kireeva, N. N.; Pastukhova, E. N. (1999). "The 74th Special Name-list of Variable Stars".Information Bulletin on Variable Stars.4659: 1.Bibcode:1999IBVS.4659....1K.

Further reading

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