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31 Persei

From Wikipedia, the free encyclopedia
Star in the constellation Perseus
31 Persei
Location of 31 Persei (circled)
Observation data
Epoch J2000      Equinox J2000
ConstellationPerseus
Right ascension03h 19m 07.63796s[1]
Declination50° 05′ 41.8724″[1]
Apparent magnitude (V)5.05[2]
Characteristics
Spectral typeB5V[3]
U−Bcolor index−0.53[4]
B−Vcolor index−0.06[4]
Astrometry
Radial velocity (Rv)−1.60[5] km/s
Proper motion (μ)RA: +23.580[1]mas/yr
Dec.: −23.322[1]mas/yr
Parallax (π)5.8399±0.1792 mas[1]
Distance560 ± 20 ly
(171 ± 5 pc)
Absolute magnitude (MV)−1.44[6]
Details
Mass4.647[7] M
Radius3.4[8] R
Luminosity950[6] L
Temperature15,301[6] K
Metallicity[Fe/H]0.00[9] dex
Rotational velocity (v sin i)260[10] km/s
Age234[11] Myr
Other designations
31 Per,BD+49°902,GC 3945,HD 20418,HIP 15444,HR 989,SAO 38714[12]
Database references
SIMBADdata

31 Persei is a single[13]star in the northernconstellation ofPerseus. It is visible to the naked eye as a dim, blue-white hued point of light with anapparent visual magnitude of 5.05.[2] This star is located around 172 parsecs (560 ly) away from the Sun,[14] and it is drifting closer with aradial velocity of −1.6 km/s.[5] It is likely a member of theAlpha Persei Cluster.[15]

This object is a massiveB-type main-sequence star with astellar classification of B5V[3] and it is currently generating energy throughhydrogen fusion at itscore. It is around 234[9] million years old and is spinning rapidly with aprojected rotational velocity of 260 km/s.[10] The star has 4.6[7] times themass of the Sun and about 3.4[8] times theradius of the Sun. It is radiating 950[6] times theluminosity of the Sun from itsphotosphere at aneffective temperature of 15,301 K.[6]

References

[edit]
  1. ^abcdeBrown, A. G. A.; et al. (Gaia collaboration) (August 2018)."Gaia Data Release 2: Summary of the contents and survey properties".Astronomy & Astrophysics.616. A1.arXiv:1804.09365.Bibcode:2018A&A...616A...1G.doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source atVizieR.
  2. ^abAnderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation".Astronomy Letters.38 (5): 331.arXiv:1108.4971.Bibcode:2012AstL...38..331A.doi:10.1134/S1063773712050015.S2CID 119257644.Vizier catalog entry
  3. ^abHoffleit, D.; Warren, W. H. (1995). "VizieR Online Data Catalog: Bright Star Catalogue, 5th Revised Ed. (Hoffleit+, 1991)".VizieR On-line Data Catalog: V/50. Originally Published in: 1964BS....C......0H.5050.Bibcode:1995yCat.5050....0H.
  4. ^abMallama, A. (2014). "Sloan Magnitudes for the Brightest Stars".The Journal of the American Association of Variable Star Observers.42 (2): 443.Bibcode:2014JAVSO..42..443M.Vizier catalog entry
  5. ^abGontcharov, G. A. (2006). "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system".Astronomy Letters.32 (11):759–771.arXiv:1606.08053.Bibcode:2006AstL...32..759G.doi:10.1134/S1063773706110065.S2CID 119231169.
  6. ^abcdeSilaj, J.; Landstreet, J. D. (2014). "Accurate age determinations of several nearby open clusters containing magnetic Ap stars".Astronomy & Astrophysics.566: A132.arXiv:1407.4531.Bibcode:2014A&A...566A.132S.doi:10.1051/0004-6361/201321468.S2CID 53370832.
  7. ^abSheikhi, Najmeh; et al. (March 2016)."The binary fraction and mass segregation in Alpha Persei open cluster".Monthly Notices of the Royal Astronomical Society.457 (1):1028–1036.arXiv:1601.02186.Bibcode:2016MNRAS.457.1028S.doi:10.1093/mnras/stw059.
  8. ^abPasinetti Fracassini, L. E.; et al. (February 2001). "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS)".Astronomy and Astrophysics.367 (2) (Third ed.):521–524.arXiv:astro-ph/0012289.Bibcode:2001A&A...367..521P.doi:10.1051/0004-6361:20000451.S2CID 425754.
  9. ^abGontcharov, G. A. (2012). "Dependence of kinematics on the age of stars in the solar neighborhood".Astronomy Letters.38 (12):771–782.arXiv:1606.08814.Bibcode:2012AstL...38..771G.doi:10.1134/S1063773712120031.S2CID 118345778.Vizier catalog entry
  10. ^abAbt, Helmut A.; et al. (2002)."Rotational Velocities of B Stars".The Astrophysical Journal.573 (1):359–365.Bibcode:2002ApJ...573..359A.doi:10.1086/340590.
  11. ^Gontcharov, G. A. (November 2012). "Spatial distribution and kinematics of OB stars".Astronomy Letters.38 (11):694–706.arXiv:1606.09028.Bibcode:2012AstL...38..694G.doi:10.1134/S1063773712110035.S2CID 119108982.
  12. ^"31 Per".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2019-07-13.
  13. ^Eggleton, P. P.; Tokovinin, A. A. (September 2008)."A catalogue of multiplicity among bright stellar systems".Monthly Notices of the Royal Astronomical Society.389 (2):869–879.arXiv:0806.2878.Bibcode:2008MNRAS.389..869E.doi:10.1111/j.1365-2966.2008.13596.x.S2CID 14878976.
  14. ^Van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction".Astronomy and Astrophysics.474 (2):653–664.arXiv:0708.1752.Bibcode:2007A&A...474..653V.doi:10.1051/0004-6361:20078357.S2CID 18759600.Vizier catalog entry
  15. ^Zuckerman, B.; et al. (June 2012). "Stellar Membership and Dusty Debris Disks in the α Persei Cluster".The Astrophysical Journal.752 (1): 12.arXiv:1204.3950.Bibcode:2012ApJ...752...58Z.doi:10.1088/0004-637X/752/1/58.S2CID 119207634. 58.
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