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Kappa Virginis

From Wikipedia, the free encyclopedia
Solitary K-type star in the constellation Virgo
κ Virginis
(Kang)
Location of κ Virginis (circled)
Observation data
EpochJ2000.0      EquinoxJ2000.0
ConstellationVirgo
Right ascension14h 12m 53.74538s[1]
Declination−10° 16′ 25.3340″[1]
Apparent magnitude (V)4.180[2]
Characteristics
Spectral typeK2/3 III[3]
U−Bcolor index+1.457[2]
B−Vcolor index+1.343[2]
Astrometry
Radial velocity (Rv)−4.38±0.21[4] km/s
Proper motion (μ)RA: +7.25[1]mas/yr
Dec.: +139.88[1]mas/yr
Parallax (π)12.80±0.25 mas[1]
Distance255 ± 5 ly
(78 ± 2 pc)
Absolute magnitude (MV)−0.28[5]
Details
Mass1.46±0.04[6] M
Radius25.41±0.74[6] R
Luminosity229[6] L
Surface gravity (log g)1.83±0.08[6] cgs
Temperature4,235±20[6] K
Metallicity[Fe/H]0.43±0.04[6] dex
Rotational velocity (v sin i)5.1[4] km/s
Age9.67±0.97[6] Gyr
Other designations
Kang, 98 Virginis,κ Vir,BD−09°3878,FK5 523,HD 124294,HIP 69427,HR 5315,SAO 158427[7]
Database references
SIMBADdata

Kappa Virginis (κ Virginis, abbreviatedKappa Vir,κ Vir), officially namedKang/ˈkæŋ/,[8] is a solitarystar in thezodiacconstellation ofVirgo. It has anapparent visual magnitude of 4.18,[2] which is sufficiently bright to be seen with the naked eye. Based uponstellar parallax measurements, the distance to this star is about 255 light-years.

Nomenclature

[edit]

κ Virginis (Latinised toKappa Virginis) is the star'sBayer designation.

InChinese,亢宿 (Kàng Sù), meaningNeck, refers to anasterism consisting of Kappa Virginis,Iota Virginis,Phi Virginis andLambda Virginis.[9] Consequently, Kappa Virginis itself is known as亢宿一 (Káng Sù yī), "the First Star of Neck".[10]

In 2016, the IAU organized aWorking Group on Star Names (WGSN)[11] to catalog and standardize proper names for stars. The WGSN approved the nameKang for this star on 30 June and it is now so included in the List of IAU-approved Star Names.[8]

Properties

[edit]

This is an orange-huedK-typegiant star with astellar classification of K2/3 III.[3] It has about 146% of themass of the Sun, but at an estimated age of 9.7 billion years it has evolved and expanded to over 25 times theSun's radius. As a consequence, it shines with around 229 times thesolar luminosity. Theeffective temperature of the star'souter atmosphere is 4,235 K.[6]

References

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  1. ^abcdevan 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.
  2. ^abcdJennens, P. A.; Helfer, H. L. (September 1975), "A new photometric metal abundance and luminosity calibration for field G and K giants",Monthly Notices of the Royal Astronomical Society,172 (3):667–679,Bibcode:1975MNRAS.172..667J,doi:10.1093/mnras/172.3.667.
  3. ^abHouk, N.; Swift, C. (1999), "Michigan catalogue of two-dimensional spectral types for the HD Stars",Michigan Spectral Survey,5,Bibcode:1999MSS...C05....0H.
  4. ^abMassarotti, Alessandro; et al. (January 2008), "Rotational and radial velocities for a sample of 761 HIPPARCOS giants and the role of binarity",The Astronomical Journal,135 (1):209–231,Bibcode:2008AJ....135..209M,doi:10.1088/0004-6256/135/1/209,S2CID 121883397.
  5. ^Anderson, 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.
  6. ^abcdefghMaldonado, J.; et al. (June 2013), "The metallicity signature of evolved stars with planets",Astronomy & Astrophysics,554: 18,arXiv:1303.3418,Bibcode:2013A&A...554A..84M,doi:10.1051/0004-6361/201321082,S2CID 119289111, A84.
  7. ^"kap Vir".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2016-09-08.
  8. ^ab"Naming Stars". IAU.org. Archived fromthe original on 10 March 2025. Retrieved16 December 2017.
  9. ^(in Chinese)中國星座神話, written by 陳久金. Published by 台灣書房出版有限公司, 2005,ISBN 978-986-7332-25-7.
  10. ^(in Chinese)香港太空館 - 研究資源 - 亮星中英對照表Archived 2008-10-25 at theWayback Machine, Hong Kong Space Museum. Accessed on line November 23, 2010.
  11. ^"IAU Working Group on Star Names (WGSN)". Archived fromthe original on 29 September 2018. Retrieved22 May 2016.
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