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39 Arietis

From Wikipedia, the free encyclopedia
Star in the constellation Aries
39 Arietis
Location of 39 Arietis (circled in red)
Observation data
Epoch J2000      Equinox J2000
ConstellationAries
Right ascension02h 47m 54.54142s[1]
Declination+29° 14′ 49.6132″[1]
Apparent magnitude (V)4.514[2]
Characteristics
Evolutionary stagered clump[3]
Spectral typeK1.5 III[4]
U−Bcolor index+1.083[2]
B−Vcolor index+1.118[2]
R−Icolor index0.58
Astrometry
Radial velocity (Rv)−15.53±0.14[5] km/s
Proper motion (μ)RA: +149.47±0.25[1]mas/yr
Dec.: −127.05±0.18[1]mas/yr
Parallax (π)19.01±0.21 mas[1]
Distance172 ± 2 ly
(52.6 ± 0.6 pc)
Details
Mass1.6[3] M
Radius10.22±0.72[6] R
Luminosity48.7±0.7[6] L
Surface gravity (log g)2.7[5] cgs
Temperature4,768±167[6] K
Metallicity[Fe/H]−0.02[5] dex
Rotational velocity (v sin i)4.5[5] km/s
Other designations
Lilii Borea,BD+28°462,HD 17361,HIP 13061,HR 824,SAO 75578.[7]
Database references
SIMBADdata

39 Arietis, officially namedLilii Borea/ˈlɪliˈbɔːriə/,[8] is astar in the northernconstellation ofAries. It is visible to the naked eye with anapparent visual magnitude of +4.5.[2] The distance to this star, as determined from an annualparallax shift of 19.01 mas,[1] is approximately 172light-years (53parsecs).This star was formerly located in the obsolete constellationMusca Borealis.

Nomenclature

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39 Arietis in optical light

39 Arietis (abbreviated39 Ari) is the star'sFlamsteed designation.

This star was described asLilii Borea byNicolas-Louis de Lacaille in 1757,[9][10] as a star of the now-defunct constellation ofLilium (theLily). The words are simply the Latin phraseLīliī Boreā 'in the north of Lilium'.Līliī Austrīnā/ɔːˈstrnə/ 'in the south of Lilium' was41 Arietis.

In 2016, theInternational Astronomical Union organized aWorking Group on Star Names (WGSN)[11] to catalog and standardize proper names for stars. The WGSN approved the nameLilii Borea for this star on 5 September 2017 and it is now so included in the List of IAU-approved Star Names.[8]

InChinese,胃宿 (Wèi Su), meaningStomach, refers to anasterism consisting of 39 Arietis,35 Arietis and41 Arietis.[12] Consequently, theChinese name for 39 Arietis itself is胃宿二 (Wèi Su èr, English:the Second Star of Stomach).[13]

Properties

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39 Arietis is agiant star with astellar classification of K1.5 III.[4] It is currently at anevolutionary stage known as thered clump, indicating that it is generating energy through the fusion ofhelium at its core.[3] It has 1.6[3] times themass of the Sun, but its outer envelope has expanded to around 10 times theSun's radius. It shines with 49 times theluminosity of the Sun. This energy is being radiated into outer space from itsouter atmosphere at aneffective temperature of 4,768 K,[6] giving it the cool orange-hued glow of aK-type star.[14]

See also

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References

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  1. ^abcdefvan Leeuwen, F. (November 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. ^abcdOja, T. (1986), "UBV photometry of stars whose positions are accurately known. III",Astronomy and Astrophysics Supplement Series,65 (2):405–4,Bibcode:1986A&AS...65..405O.
  3. ^abcdTautvaišienė, G.; et al. (December 2010), "C, N and O abundances in red clump stars of the Milky Way",Monthly Notices of the Royal Astronomical Society,409 (3):1213–1219,arXiv:1007.4064,Bibcode:2010MNRAS.409.1213T,doi:10.1111/j.1365-2966.2010.17381.x,S2CID 119182458.
  4. ^abNordgren, Tyler E.; et al. (December 1999),"Stellar Angular Diameters of Late-Type Giants and Supergiants Measured with the Navy Prototype Optical Interferometer",The Astronomical Journal,118 (6):3032–3038,Bibcode:1999AJ....118.3032N,doi:10.1086/301114
  5. ^abcdMassarotti, 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.
  6. ^abcdBaines, Ellyn K.; Clark, James H.; Schmitt, Henrique R.; Stone, Jordan M.; von Braun, Kaspar (2023-12-01), "33 New Stellar Angular Diameters from the NPOI, and Nearly 180 NPOI Diameters as an Ensemble",The Astronomical Journal,166 (6): 268,arXiv:2505.23514,Bibcode:2023AJ....166..268B,doi:10.3847/1538-3881/ad08be,ISSN 0004-6256
  7. ^"* 39 Ari".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2012-07-18.
  8. ^ab"Naming Stars". IAU.org. Retrieved16 December 2017.
  9. ^de Lacaille, Nicolas-Louis (1757).Astronomiae fundamenta novissimis solis et stellarum observationibus stabilita, Lutetiae in Collegio mazarineo et in Africa ad caput Bonae Spei peractis a Nicolao Ludovico de La Caille. J.-J.-St. Collombat. pp. 227, 233.
  10. ^Baily, Francis (1833).La Caille's Catalogue of 398 principal Stars, Memoirs of the Royal Astronomical Society, Vol 5. Priestley and Weale. pp. 110, 121.
  11. ^"IAU Working Group on Star Names (WGSN)". Retrieved22 May 2016.
  12. ^(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.
  13. ^(in Chinese)白羊座
  14. ^"The Colour of Stars",Australia Telescope, Outreach and Education,Commonwealth Scientific and Industrial Research Organisation, December 21, 2004, archived fromthe original on February 22, 2012, retrieved2012-01-16

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