11 Andromedae
Observation data EpochJ2000EquinoxJ2000 | |
---|---|
Constellation | Andromeda |
Right ascension | 23h19m29.80701s[1] |
Declination | +48° 37′ 31.1615″[1] |
Apparent magnitude(V) | 5.44[2] |
Characteristics | |
Spectral type | K0 III[3] |
U−Bcolor index | +0.82[4] |
B−Vcolor index | +1.014±0.003[2] |
Astrometry | |
Radial velocity(Rv) | +9.99±0.14[1]km/s |
Proper motion(μ) | RA:+22.597[1]mas/yr Dec.:+52.689[1]mas/yr |
Parallax(π) | 11.5097 ± 0.0858mas[1] |
Distance | 283 ± 2ly (86.9 ± 0.6pc) |
Absolute magnitude(MV) | 0.73[2] |
Details | |
Mass | 2.57[5]M☉ |
Radius | 12[6]R☉ |
Luminosity | 62.86[2]L☉ |
Surface gravity(logg) | 2.61[5]cgs |
Temperature | 4,874[5]K |
Metallicity[Fe/H] | −0.13±0.07[7]dex |
Rotational velocity(vsini) | 1.0[8]km/s |
Other designations | |
Database references | |
SIMBAD | data |
11 Andromedae,abbreviated11 And,is a single,[10]orange-huedstarin the northernconstellationofAndromeda.11 Andromedaeis theFlamsteed designation.It has anapparent visual magnitudeof 5.44,[2]which is bright enough to be faintly visible to the naked eye. An annualparallax shiftof11.5mas[1]yields a distance estimate of 283light years.It is moving further from the Earth with a heliocentricradial velocityof +10 km/s.[1]
This is anevolvedgiant starwith astellar classificationof K0 III,[3]which means it has exhausted the supply of hydrogen at its core and turned off themain sequence.It has an estimated 2.57[5]times themass of the Sunand has expanded to around 12[6]times theSun's radius.It is radiating 63[2]times theSun's luminosityfrom its enlargedphotosphereat aneffective temperatureof 4,874 km/s.[5]
Within Andromeda it is the south-west end of a bright northerly chain (jagged line)asterism– the others being, their order going with numbering, 8, 7, 5 and3 Andromedae.
References
[edit]- ^abcdefghBrown, A. G. A.;et al. (Gaia collaboration) (August 2018)."GaiaData 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.
- ^abcdefAnderson, 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,S2CID119257644.
- ^abGriffin, R. F.; Redman, R. O. (1960), "Photoelectric measurements of the lambda 4200 A CN band and the G band in G8-K5 spectra",Monthly Notices of the Royal Astronomical Society,120:287,Bibcode:1960MNRAS.120..287G,doi:10.1093/mnras/120.4.287.
- ^Hoffleit, D.; Warren Jr., W. H., "HR 8874, database entry",The Bright Star Catalogue(5th Revised (Preliminary Version) ed.),CDS.IDV/50.Accessed on line August 21, 2008.
- ^abcdeLiu, Y. J.; et al. (April 2014), "The Lithium Abundances of a Large Sample of Red Giants",The Astrophysical Journal,785(2): 12,arXiv:1404.1687,Bibcode:2014ApJ...785...94L,doi:10.1088/0004-637X/785/2/94,S2CID119226316,94.
- ^abPasinetti Fracassini, L. E.; Pastori, L.; Covino, S.; Pozzi, A. (February 2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS)",Astronomy and Astrophysics,367(Third ed.): 521–524,arXiv:astro-ph/0012289,Bibcode:2001A&A...367..521P,doi:10.1051/0004-6361:20000451,S2CID425754
- ^Gáspár, András; et al. (2016), "The Correlation between Metallicity and Debris Disk Mass",The Astrophysical Journal,826(2): 171,arXiv:1604.07403,Bibcode:2016ApJ...826..171G,doi:10.3847/0004-637X/826/2/171,S2CID119241004.
- ^De Medeiros, J. R.; et al. (November 2000), "Rotation and lithium in single giant stars",Astronomy and Astrophysics,363:239–243,arXiv:astro-ph/0010273,Bibcode:2000A&A...363..239D.
- ^"11 And".SIMBAD.Centre de données astronomiques de Strasbourg.RetrievedSeptember 18,2018.
- ^Eggleton, P. P.; Tokovinin, A. A. (September 2008), "A catalogue of multiplicity among bright stellar systems",Monthly Notices of the Royal Astronomical Society,389(2): 869–879,arXiv:0806.2878,Bibcode:2008MNRAS.389..869E,doi:10.1111/j.1365-2966.2008.13596.x,S2CID14878976.