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49 Andromedae

From Wikipedia, the free encyclopedia
Star in the constellation Andromeda
This article is about A Andromedae; it is not to be confused withα Andromedae.
49 Andromedae
Location of 49 Andromedae (circled)
Observation data
Epoch J2000      Equinox J2000
ConstellationAndromeda[1]
Right ascension01h 30m 06.10151s[2]
Declination+47° 00′ 26.1811″[2]
Apparent magnitude (V)5.269[3]
Characteristics
Evolutionary stagered clump[4]
Spectral typeK0 III[5]
B−Vcolor index0.993[3]
Astrometry
Radial velocity (Rv)−11.48[3] km/s
Proper motion (μ)RA: −0.950mas/yr[2]
Dec.: −42.638mas/yr[2]
Parallax (π)9.7947±0.1166 mas[2]
Distance333 ± 4 ly
(102 ± 1 pc)
Absolute magnitude (MV)0.50[1]
Details
Mass2.07[3] M
Radius11[6] R
Luminosity70.8[3] L
Surface gravity (log g)2.30[4] cgs
Temperature4,879±106[3] K
Metallicity[Fe/H]+0.020±0.04[4] dex
Rotational velocity (v sin i)2.0[7] km/s
Age1.75[3] Gyr
Other designations
a And[8],49 And,BD+46°370,HD 9057,HIP 6999,HR 430,SAO 37275,PPM 44057,GSC 03282-02272[9]
Database references
SIMBADdata

49 Andromedae is astar in theconstellationAndromeda.[1]49 Andromedae is theFlamsteed designation (abbreviated49 And),[9] though it also bears theBayer designationa Andromedae.[8] It is visible to thenaked eye under good viewing conditions with anapparent visual magnitude of 5.269.[3] The distance to 49 Andromedae, as determined from its annualparallax shift of9.8 mas,[2] is around 333 light-years. It is drifting closer to theSun with a heliocentricradial velocity of −11.5 km/s.[3]

With an estimated age of1.75 Gyr[3] years, this is an agingred-clump[4]giant star with astellar classification of K0 III,[5] indicating it is generating energy byhelium fusion at itscore. Thespectrum displays "slightly strong"absorption lines ofcyanogen (CN).[5] It has 2.07[3] times themass of the Sun and has expanded to 11[6] times theSun's radius. The star is radiating 71[3] times theSun's luminosity from its enlargedphotosphere at aneffective temperature of4,879 K.[3] It is spinning with aprojected rotational velocity of2 km/s.[7]

This was one of the stars historically known asAdhil, from Arabicað-ðayl "thetrain [of a garment]", a name now applied toξ Andromedae.[10] In a 1971 NASA technical memorandum listing star names, 49 Andromedae was listed asThail, likely derived from the same Arabic name.[11]

References

[edit]
  1. ^abcAnderson, 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.
  2. ^abcdeVallenari, 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.
  3. ^abcdefghijklmLuck, 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.
  4. ^abcdTautvaišienė, G.; et al. (March 2013), "Red clump stars of the Milky Way - laboratories of extra-mixing",Monthly Notices of the Royal Astronomical Society,430 (1): 621−627,arXiv:1304.4393,Bibcode:2013MNRAS.430..621T,doi:10.1093/mnras/sts663,S2CID 119211439.
  5. ^abcSchmitt, John L. (January 1971), "Stars with Strong Cyanogen Absorption",Astrophysical Journal,163: 75,Bibcode:1971ApJ...163...75S,doi:10.1086/150747.
  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,S2CID 121883397.
  7. ^abDe 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.
  8. ^abTirion, W.; et al. (1987), Willmann-Bell, Inc. (ed.),Uranometria 2000.0 - Volume II - The Southern Hemisphere to +6°, Richmond, Virginia, USA,ISBN 0-943396-15-8.
  9. ^ab"49 And".SIMBAD.Centre de données astronomiques de Strasbourg. RetrievedOctober 1, 2018.
  10. ^Allen, R.H. (1899),Star Names: Their Lore and Meaning, p. 38-39
  11. ^Rhoads, Jack W. (November 15, 1971),Technical Memorandum 33-507-A Reduced Star Catalog Containing 537 Named Stars(PDF), Jet Propulsion Laboratory, California Institute of Technology.
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