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4 Andromedae

From Wikipedia, the free encyclopedia
Star in the constellation Andromeda
Not to be confused withAndromeda IV.
4 Andromedae
Location of 4 Andromedae (circled)
Observation data
Epoch J2000      Equinox J2000
ConstellationAndromeda
Right ascension23h 07m 39.2672s[1]
Declination+46° 23′ 14.030″[1]
Apparent magnitude (V)5.308[2]
Characteristics
Evolutionary stageGiant star
Spectral typeK5 III[3]
B−Vcolor index1.436[2]
Astrometry
Radial velocity (Rv)−11.89±0.12[1] km/s
Proper motion (μ)RA: −12.734mas/yr[1]
Dec.: −30.026mas/yr[1]
Parallax (π)9.155±0.0779 mas[1]
Distance356 ± 3 ly
(109.2 ± 0.9 pc)[1]
Details
Mass1.58±0.44[4] M
Radius23.36±0.59[5] R
Luminosity170[6] L
Surface gravity (log g)1.91[2] cgs
Temperature4,275±92[4] K
Metallicity[Fe/H]1.98±0.11[4] dex
Age2.24+0.78
−0.58
[4] Gyr
Other designations
4 And,BD+45°4149,FK5 3852,HD 218452,HIP 114200,HR 8804,SAO 52711,PPM 63840,WDS J23077+4623A[7]
Database references
SIMBADdata

4 Andromedae, abbreviated4 And, is a single[8]star in the northernconstellation ofAndromeda.4 Andromedae is theFlamsteed designation. It is dimly visible to the naked eye with anapparent visual magnitude of 5.308.[2] Based upon an annualparallax shift of9.16 mas[1] as seen from Earth's orbit, it is located 356 light years away. At this distance,interstellar extinction diminishes the apparent magnitude of 4 And by 0.5326magnitudes.[1] The star is moving closer with a heliocentricradial velocity of −11 km/s.[9] It has a magnitude 11.7visual companion at anangular separation of51.10 along aposition angle of 348°, as of 2002.[10]

At the age of 2.2[4] billion years, this is an aginggiant star with astellar classification of K5 III,[3] having consumed the hydrogen at its core andevolved away from themain sequence. It has 1.6[4] times themass of the Sun and has expanded to 23[5] times theSun's radius. The star is radiating 170[6] times theSun's luminosity from its enlargedphotosphere at aneffective temperature of 4,275 K.[4]

References

[edit]
  1. ^abcdefghVallenari, 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. ^abcdSoubiran, Caroline; et al. (2016), "The PASTEL catalogue: 2016 version",Astronomy & Astrophysics,591: A118,arXiv:1605.07384,Bibcode:2016A&A...591A.118S,doi:10.1051/0004-6361/201628497,S2CID 119258214.
  3. ^abEggen, O. J. (1962), "Space-velocity vectors for 3483 stars with proper motion and radial velocity",Royal Observatory Bulletin,51: 79,Bibcode:1962RGOB...51...79E.
  4. ^abcdefgFeuillet, 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.
  5. ^abBaines, Ellyn K.; Thomas Armstrong, J.; Clark, James H.; Gorney, Jim; Hutter, Donald J.; Jorgensen, Anders M.; Kyte, Casey; Mozurkewich, David; Nisley, Ishara; Sanborn, Jason; Schmitt, Henrique R.; Van Belle, Gerard T. (2021)."Angular Diameters and Fundamental Parameters of Forty-four Stars from the Navy Precision Optical Interferometer".The Astronomical Journal.162 (5): 198.arXiv:2211.09030.Bibcode:2021AJ....162..198B.doi:10.3847/1538-3881/ac2431.
  6. ^abAurière, M.; et al. (February 2015), "The magnetic fields at the surface of active single G-K giants",Astronomy & Astrophysics,574: 30,arXiv:1411.6230,Bibcode:2015A&A...574A..90A,doi:10.1051/0004-6361/201424579,S2CID 118504829, A90.
  7. ^"4 And".SIMBAD.Centre de données astronomiques de Strasbourg. RetrievedSeptember 12, 2018.
  8. ^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.
  9. ^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.
  10. ^Mason, B. D.; et al. (2014),"The Washington Visual Double Star Catalog",The Astronomical Journal,122 (6): 3466,Bibcode:2001AJ....122.3466M,doi:10.1086/323920, retrieved2015-07-22.

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