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Lambda Persei

From Wikipedia, the free encyclopedia
Star in the constellation Perseus
Lambda Persei
Location of λ Persei (circled)
Observation data
Epoch J2000      Equinox J2000
ConstellationPerseus
Right ascension04h 06m 35.04360s[1]
Declination+50° 21′ 04.5500″[1]
Apparent magnitude (V)4.29[2]
Characteristics
Spectral typeA0IVn[3]
U−Bcolor index−0.04[2]
B−Vcolor index+0.02[2]
Astrometry
Radial velocity (Rv)+6.1±2.0[4] km/s
Proper motion (μ)RA: −12.75[1]mas/yr
Dec.: −35.60[1]mas/yr
Parallax (π)7.73±0.22 mas[1]
Distance420 ± 10 ly
(129 ± 4 pc)
Absolute magnitude (MV)−1.31[5]
Details
Radius3.1[6] R
Luminosity348[5] L
Surface gravity (log g)4.05[7] cgs
Temperature10,585[7] K
Metallicity[Fe/H]+0.01[7] dex
Rotational velocity (v sin i)196[8] km/s
Age345[9] Myr
Other designations
λ Per,47 Persei,BD+49°1101,FK5 1113,GC 4924,HD 25642,HIP 19167,HR 1261,SAO 24412[10]
Database references
SIMBADdata

λ Persei,Latinized asLambda Persei, is astar in the northernconstellation ofPerseus. It is visible to the naked eye as a faint, white-hued point of light with anapparent visual magnitude of 4.29.[2] This object is located approximately 422 light years from the Sun based onparallax,[1] and is drifting further away with aradial velocity of +6 km/s.[4]

λ Persei in optical light

This object has astellar classification of A0IVn,[3] matching anA-typesubgiant star with "nebulous"lines due to rapid rotation. It is spinning with aprojected rotational velocity of 196 km/s,[8] which is giving the star anequatorial bulge that is an estimated 16% larger than the polar radius.[11] Unusually for a star of this type,spectra show weakemission features among theHydrogen lines, which may be due toplage regions on the surface caused by an impliedmagnetic field.[12] The star is 345[9] million years old and is radiating 348[5] times theluminosity of the Sun from itsphotosphere at aneffective temperature of 10,585 K.[7]

InChinese astronomy, Lambda Persei is called 積水,Pinyin: Jīshuǐ, meaningStored Water, because this star is marking itself and stand alone inStored Water asterism,Stomach mansion (see :Chinese constellation).[13] This name has also been applied toOmicron Geminorum and was approved by theIAU Working Group on Star Names as the name of that star.[14]

References

[edit]
  1. ^abcdefVan 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
  2. ^abcdDucati, J. R. (2002). "Catalogue of Stellar Photometry in Johnson's 11-color system".CDS/ADC Collection of Electronic Catalogues.2237.Bibcode:2002yCat.2237....0D.
  3. ^abCowley, A.; et al. (April 1969). "A study of the bright A stars. I. A catalogue of spectral classifications".Astronomical Journal.74:375–406.Bibcode:1969AJ.....74..375C.doi:10.1086/110819.
  4. ^abWilson, R. E. (1953). "General Catalogue of Stellar Radial Velocities".Carnegie Institute Washington D.C. Publication.Carnegie Institution for Science.Bibcode:1953GCRV..C......0W.LCCN 54001336.
  5. ^abcAnderson, 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
  6. ^Pasinetti 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
  7. ^abcdWu, Yue; et al. (2010). "Coudé-feed stellar spectral library – atmospheric parameters".Astronomy & Astrophysics.525: A71.arXiv:1009.1491.Bibcode:2011A&A...525A..71W.doi:10.1051/0004-6361/201015014.S2CID 53480665.
  8. ^abHoffleit, D.; Warren, W. H. (1995). "Bright Star Catalogue".VizieR On-line Data Catalog: V/50. Originally Published in: 1964BS....C......0H.5050 (5th Revised ed.).Bibcode:1995yCat.5050....0H.
  9. ^abGontcharov, 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.
  10. ^"lam Per".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2019-09-22.
  11. ^Belle, G. T. (2012). "Interferometric observations of rapidly rotating stars".The Astronomy and Astrophysics Review.20 (1): 51.arXiv:1204.2572.Bibcode:2012A&ARv..20...51V.doi:10.1007/s00159-012-0051-2.S2CID 119273474.
  12. ^Underhill, Anne B. (November 1991). "Lambda Persei: an Unusual B9 IV Star".Publications of the Astronomical Society of the Pacific.103: 1176.Bibcode:1991PASP..103.1176U.doi:10.1086/132937.S2CID 121711589.
  13. ^(in Chinese)AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 7 月 11 日Archived 2012-02-04 at theWayback Machine
  14. ^"IAU Catalog of Star Names". Retrieved22 February 2025.
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