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51 Andromedae

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51 Andromedae
Observation data
Epoch J2000      Equinox J2000
Constellation Andromeda
Right ascension 01h 37m 59.56074s[1]
Declination +48° 37′ 41.5798″[1]
Apparent magnitude (V) 3.57[2]
Characteristics
Spectral type K3- III CN0.5[3]
U−B color index +1.44[2]
B−V color index +1.28[2]
Astrometry
Radial velocity (Rv)18.41[4] km/s
Proper motion (μ) RA: +61.334[1] mas/yr
Dec.: -113.100[1] mas/yr
Parallax (π)19.2489 ± 0.4077 mas[1]
Distance169 ± 4 ly
(52 ± 1 pc)
Absolute magnitude (MV)−0.04[5]
Details[6]
Mass1.75±0.15 M☉
Radius21.30±0.21 R☉
Luminosity142.1±7.6 L☉
Surface gravity (log g)2.01 cgs
Temperature4,951±64 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[7]
Database references
SIMBADdata

51 Andromedae, abbreviated 51 And and also named Nembus,[8] is the 5th brightest (4th magnitude) star in the northern constellation of Andromeda. It is an orange K-type giant star with an apparent magnitude of +3.59 and is approximately 169 light-years from the Earth.

At an estimated age of 1.7 billion years, this is an evolved red giant star with a stellar classification of K3- III CN0.5.[3] The suffix notation indicates a mild enhancement of cyanogen absorption lines in its spectrum. This star has 1.8 times the mass of the Sun and it has expanded to 21.3 times the Sun's radius. It is radiating 142 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,951 K.[6]

Nomenclature

51 Andromedae is the star's Flamsteed designation. (Ptolemy included this star in Andromeda in the Almagest, but it was moved into Perseus by Johann Bayer, who designated it Upsilon Persei. Flamsteed moved it back, and the International Astronomical Union (IAU) made Flamsteed's 51 Andromedae its official designation in 1930.[9][10][11])

The star bore the traditional name Nembus[12] in Bayer's Uranometria (1603)[13] and Bode's star atlas Uranographia (1801).[14] In 2016, the IAU organized a Working Group on Star Names (WGSN)[15] to catalog and standardize proper names for stars. The WGSN approved the name Nembus for this star on 5 September 2017 and it is now so included in the List of IAU-approved Star Names.[8]

In Chinese, 天大將軍 (Tiān Dà Jiāng Jūn), meaning Heaven's Great General, refers to an asterism consisting of 51 Andromedae, Gamma Andromedae, Phi Persei, 49 Andromedae, Chi Andromedae, Upsilon Andromedae, Tau Andromedae, 56 Andromedae, Beta Trianguli, Gamma Trianguli and Delta Trianguli.[16] Consequently, 51 Andromedae itself is known as 天大將軍三 (Tiān Dà Jiāng Jūn sān, Template:Lang-en.)[17]

References

  1. ^ a b c d e Brown, 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.
  2. ^ a b c Ducati, 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.
  3. ^ a b Keenan, 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.
  4. ^ 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.
  5. ^ 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.
  6. ^ a b Baines, Ellyn K.; et al. (2018), "Fundamental Parameters of 87 Stars from the Navy Precision Optical Interferometer", The Astronomical Journal, 155, 30, arXiv:1712.08109, Bibcode:2018AJ....155...30B, doi:10.3847/1538-3881/aa9d8b.{{citation}}: CS1 maint: unflagged free DOI (link)
  7. ^ "HD 9927". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 24 August 2018.
  8. ^ a b "Naming Stars". IAU.org. Retrieved 16 December 2017.
  9. ^ "Ephemerides – Report of Commissions", Transactions of the International Astronomical Union, 4: 20, 1932
  10. ^ Allen, R. H. (1899). Star-names and Their Meanings. New York: G. E. Stechart., p.34.
  11. ^ Wagman, Morton (2003) Lost Stars p.240, McDonald and Woodward, Blacksburg, Virginia. ISBN 0-939923-78-5.
  12. ^ Allen, R. H. (1899). Star-names and Their Meanings. New York: G. E. Stechart. p.334
  13. ^ Scans of the plates of Uranometria by J. Bayer, 1603 Archived August 7, 2008, at the Wayback Machine @Linda Hall Library
  14. ^ Scan of the plates of Uranographia by J.E. Bode, 1801 @Ian Ridpath's Star Tales
  15. ^ "IAU Working Group on Star Names (WGSN)". Retrieved 22 May 2016.
  16. ^ Template:Zh icon 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.
  17. ^ Template:Zh icon http://zh.wikipedia.org/zh-tw/%E5%A4%A9%E5%A4%A7%E5%B0%86%E5%86%9B%E4%B8%89
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