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51 Andromedae

From Wikipedia, the free encyclopedia
Red giant star in the constellation Andromeda
51 Andromedae
Location of 51 Andromedae (circled)
Observation data
Epoch J2000      Equinox J2000
ConstellationAndromeda[1]
Right ascension01h 37m 59.56074s[2]
Declination+48° 37′ 41.5798″[2]
Apparent magnitude (V)3.57[3]
Characteristics
Spectral typeK3- III CN0.5[4]
U−Bcolor index+1.44[3]
B−Vcolor index+1.28[3]
Astrometry
Radial velocity (Rv)18.41[5] km/s
Proper motion (μ)RA: +61.334[2]mas/yr
Dec.: -113.100[2]mas/yr
Parallax (π)19.2489±0.4077 mas[2]
Distance169 ± 4 ly
(52 ± 1 pc)
Absolute magnitude (MV)−0.04[6]
Details[7]
Mass1.75±0.15 M
Radius21.30±0.21 R
Luminosity142.1±7.6 L
Surface gravity (log g)2.01 cgs
Temperature4,316±54 K
Metallicity[Fe/H]0.07 dex
Age1.70±0.40 Gyr
Other designations
υ Per,51 And,BD+47°467,HD 9927,HIP 7607,HR 464,SAO 37375,PPM 44238[8]
Database references
SIMBADdata

51 Andromedae, abbreviated51 And and formally namedNembus/ˈnɛmbəs/,[9] is the 5th brighteststar in the northernconstellation ofAndromeda, very slightly dimmer than theAndromeda Galaxy also being of 4thmagnitude. It is an orangeK-typegiant star with anapparent magnitude of +3.57 and is about 169light-years from theEarth/solar system. It is traditionally depicted as one of the two northern, far upper ends of the mythological, chained-to-the-rocks princess, the other being binary star systemGamma Andromedae.

At an estimated age of 1.7 billion years, this is anevolvedred giant star with astellar classification ofK3- III CN0.5.[4] The suffix notation indicates a mild enhancement ofcyanogenabsorption lines in itsspectrum. This star has 1.8 times themass of the Sun and it has expanded to 21.3 times theSun's radius. It is radiating 142 times theSun's luminosity from its enlargedphotosphere at aneffective temperature of 4,951 K.[7]

Nomenclature

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51 Andromedae is the star'sFlamsteed designation.Ptolemy included this star in Andromeda in theAlmagest. It was for a time moved into the greater form of Perseus envisioned byJohann Bayer asUpsilon Persei.Flamsteed oversaw its constellation reverting and theInternational Astronomical Union (IAU) made his51 Andromedae its official designation in 1930.[10][11][12]

The star bore the nameNembus, of undetermined origin and meaning,[13] in Bayer'sUranometria (1603)[14] andBode'sstar atlasUranographia (1801).[15] In 2016, the IAU organized aWorking Group on Star Names (WGSN)[16] to catalog and standardize proper names for stars. The WGSN approved the nameNembus for this star on 5 September 2017 and it is now so included in the List of IAU-approved Star Names.[9]

InChinese,天大將軍 (Tiān Dà Jiāng Jūn), meaningHeaven's Great General, refers to anasterism consisting of 51 Andromedae,Gamma Andromedae,Phi Persei,49 Andromedae,Chi Andromedae,Upsilon Andromedae,Tau Andromedae,56 Andromedae,Beta Trianguli,Gamma Trianguli andDelta Trianguli.[17] Consequently, theChinese name for 51 Andromedae itself is天大將軍三 (Tiān Dà Jiāng Jūn sān, English:the Third Star of Heaven's Great General.)[citation needed]

References

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  1. ^Roman, Nancy G. (1987)."Identification of a constellation from a position".Publications of the Astronomical Society of the Pacific.99 (617): 695.Bibcode:1987PASP...99..695R.doi:10.1086/132034. Constellation record for this object atVizieR.
  2. ^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.
  3. ^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.
  4. ^abKeenan, Philip C.; McNeil, Raymond C. (1989). "The Perkins catalog of revised MK types for the cooler stars".Astrophysical Journal Supplement Series.71: 245.Bibcode:1989ApJS...71..245K.doi:10.1086/191373.
  5. ^Maldonado, J.; Villaver, E.; Eiroa, C. (2013). "The metallicity signature of evolved stars with planets".Astronomy & Astrophysics.554: A84.arXiv:1303.3418.Bibcode:2013A&A...554A..84M.doi:10.1051/0004-6361/201321082.S2CID 119289111.
  6. ^Cardini, D. (January 2005), "Mg II chromospheric radiative loss rates in cool active and quiet stars",Astronomy and Astrophysics,430:303–311,arXiv:astro-ph/0409683,Bibcode:2005A&A...430..303C,doi:10.1051/0004-6361:20041440,S2CID 12136256.
  7. ^abBaines, Ellyn K.; et al. (2018), "Fundamental Parameters of 87 Stars from the Navy Precision Optical Interferometer",The Astronomical Journal,155 (1), 30,arXiv:1712.08109,Bibcode:2018AJ....155...30B,doi:10.3847/1538-3881/aa9d8b,S2CID 119427037.
  8. ^"HD 9927".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved24 August 2018.
  9. ^ab"Naming Stars". IAU.org. Retrieved16 December 2017.
  10. ^"Ephemerides – Report of Commissions",Transactions of the International Astronomical Union,4: 20, 1932
  11. ^Allen, R. H. (1899).Star-names and Their Meanings. New York: G. E. Stechart., p.34.
  12. ^Wagman, Morton (2003)Lost Stars p.240, McDonald and Woodward, Blacksburg, Virginia.ISBN 0-939923-78-5.
  13. ^Allen, R. H. (1899).Star-names and Their Meanings. New York: G. E. Stechart. p.334
  14. ^Scans of the plates ofUranometria by J. Bayer, 1603Archived August 7, 2008, at theWayback Machine @Linda Hall Library
  15. ^Scan of the plates ofUranographia by J.E. Bode, 1801 @Ian Ridpath'sStar Tales
  16. ^"IAU Working Group on Star Names (WGSN)". Retrieved22 May 2016.
  17. ^(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.

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