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3 Andromedae

From Wikipedia, the free encyclopedia
Star in the constellation Andromeda
Not to be confused withAndromeda III.
3 Andromedae
Location of 3 Andromedae (circled)
Observation data
Epoch J2000      Equinox J2000
ConstellationAndromeda
Right ascension23h 04m 10.98269s[1]
Declination+50° 03′ 07.5255″[1]
Apparent magnitude (V)4.64[2]
Characteristics
Evolutionary stagegiant[3]
Spectral typeK0 IIIb[4]
B−Vcolor index1.058±0.003[2]
Astrometry
Radial velocity (Rv)−34.87±0.12[1] km/s
Proper motion (μ)RA: 165.837[1]mas/yr[1]
Dec.: 167.716mas/yr[1]
Parallax (π)17.2629±0.0918 mas[1]
Distance189 ± 1 ly
(57.9 ± 0.3 pc)
Absolute magnitude (MV)0.97[2]
Details
Mass1.71[5] M
Radius10[6] R
Luminosity49[5] L
Surface gravity (log g)2.61±0.11[7] cgs
Temperature4,668±45[5] K
Metallicity [Fe/H]−0.08[3] dex
Rotational velocity (v sin i)1.0[8] km/s
Age2.27[5] Gyr
Other designations
3 And,BD+49°4028,HD 218031,HIP 113919,HR 8780,SAO 52649,PPM 41448,LTT 16772[9]
Database references
SIMBADdata

3 Andromedae, abbreviated3 And, is a single[10]star in the northernconstellation ofAndromeda.3 Andromedae is theFlamsteed designation. It is visible to the naked eye with anapparent visual magnitude of 4.64.[2] The distance to this star, as determined from an annualparallax shift of17.3 mas,[1] is 181 light years. It is moving closer to the Earth with a heliocentricradial velocity of −35 km/s,[11] and has a relatively largeproper motion, traversing thecelestial sphere at0.236·yr−1.[12]

This is anevolvedgiant star with astellar classification of K0 IIIb,[4] where the 'b' suffix indicated a lower luminosity giant. It is ared clump star,[3] which means it is generating energy throughhelium fusion at itscore. This star has an estimated 1.7[5] times themass of the Sun (M), and, at the age of 2.3[5] billion years, has expanded to 10 times theSun's radius (R).[6] It is radiating 49[5] times theSun's luminosity from its enlargedphotosphere at aneffective temperature of 4,668 K.[5]

References

[edit]
  1. ^abcdefgVallenari, A.; et al. (Gaia collaboration) (2023)."Gaia Data Release 3. Summary of the content and survey properties".Astronomy and Astrophysics.674: A1.arXiv:2208.00211.Bibcode:2023A&A...674A...1G.doi:10.1051/0004-6361/202243940.S2CID 244398875. Gaia DR3 record for this source atVizieR.
  2. ^abcdAnderson, 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.
  3. ^abcTautvaišienė, 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. ^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. ^abcdefghLuck, R. Earle (2015), "Abundances in the Local Region. I. G and K Giants",Astronomical Journal,150 (3), 88,arXiv:1507.01466,Bibcode:2015AJ....150...88L,doi:10.1088/0004-6256/150/3/88,S2CID 118505114.
  6. ^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.
  7. ^Feuillet, Diane K.; et al. (2016), "Determining Ages of APOGEE Giants with Known Distances",The Astrophysical Journal,817 (1): 40,arXiv:1511.04088,Bibcode:2016ApJ...817...40F,doi:10.3847/0004-637X/817/1/40,S2CID 118675933.
  8. ^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.
  9. ^"3 And".SIMBAD.Centre de données astronomiques de Strasbourg. RetrievedSeptember 12, 2018.
  10. ^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,S2CID 14878976.
  11. ^Gontcharov, G. A. (2006), "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system",Astronomy Letters,32 (11):759–771,arXiv:1606.08053,Bibcode:2006AstL...32..759G,doi:10.1134/S1063773706110065,S2CID 119231169.
  12. ^Lépine, Sébastien; Shara, Michael M. (March 2005), "A Catalog of Northern Stars with Annual Proper Motions Larger than 0.15" (LSPM-NORTH Catalog)",The Astronomical Journal,129 (3):1483–1522,arXiv:astro-ph/0412070,Bibcode:2005AJ....129.1483L,doi:10.1086/427854,S2CID 2603568.
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