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22 Andromedae

From Wikipedia, the free encyclopedia
Star in the constellation Andromeda
22 Andromedae
Location of 22 Andromedae (circled)
Observation data
Epoch J2000      Equinox J2000
ConstellationAndromeda
Right ascension00h 10m 19.24653s[1]
Declination+46° 04′ 20.1704″[1]
Apparent magnitude (V)5.04[2]
Characteristics
Spectral typeF5 II[3] orF5 Ib–II metal-weak[4]
B−Vcolor index+0.04[2]
Astrometry
Radial velocity (Rv)−8.2±2.2[5] km/s
Proper motion (μ)RA: 5.472[1]mas/yr
Dec.: 0.086[1]mas/yr
Parallax (π)2.2233±0.3881 mas[1]
Distanceapprox. 1,500 ly
(approx. 450 pc)
Absolute magnitude (MV)−3.51[6]
Details
Mass6.1±0.4[3] M
Radius17[7] R
Luminosity1,436[8] L
Surface gravity (log g)2.10±0.08[3] cgs
Temperature6,270±150[3] K
Metallicity[Fe/H]−0.09±0.05[2] dex
Rotational velocity (v sin i)46[9] km/s
Age62[3] Myr
Other designations
22 And,BD+45°17,FK5 4,HD 571,HIP 841,HR 27,SAO 36123,PPM 42645[10]
Database references
SIMBADdata

22 Andromedae, abbreviated22 And, is a single[11]star in theconstellationAndromeda.22 Andromedae is theFlamsteed designation. It is visible to the naked eye with anapparent visual magnitude of 5.04.[2] The distance to 22 And can be estimated from its annualparallax shift of just2.2 mas,[1] which shows it to be around 1,500 light years away. It is moving closer to the Earth with a heliocentricradial velocity of −8.2 km/s.[5]

This is abright giant with astellar classification of F5 II.[3] Gray et al. (2001) classify it as F5 Ib–IImetal-weak, with the metalliclines matching a class of F0 whereas hydrogen lines match an F5.[4] It is around 62[3] million years old with aprojected rotational velocity of 46 km/s.[9] The star has six[3] times themass of the Sun and has expanded to about 17[7] times theSun's radius. It is radiating 1,436[8] times theSun's luminosity from itsphotosphere at aneffective temperature of 6,270 km/s.[3]

References

[edit]
  1. ^abcdefBrown, 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. ^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. ^abcdefghiLyubimkov, Leonid S.; et al. (2010), "Accurate fundamental parameters for A-, F- and G-type Supergiants in the solar neighbourhood",Monthly Notices of the Royal Astronomical Society,402 (2):1369–79,arXiv:0911.1335,Bibcode:2010MNRAS.402.1369L,doi:10.1111/j.1365-2966.2009.15979.x,S2CID 119096173.
  4. ^abGray, R. O.; et al. (2001), "The Physical Basis of Luminosity Classification in the Late A-, F-, and Early G-Type Stars. I. Precise Spectral Types for 372 Stars",The Astronomical Journal,121 (4): 2148,Bibcode:2001AJ....121.2148G,doi:10.1086/319956.
  5. ^abde Bruijne, J. H. J.; Eilers, A.-C. (October 2012), "Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project",Astronomy & Astrophysics,546: 14,arXiv:1208.3048,Bibcode:2012A&A...546A..61D,doi:10.1051/0004-6361/201219219,S2CID 59451347, A61.
  6. ^Kovtyukh, V. V.; et al. (2012), "Accurate luminosities from the oxygen λ7771-4 Å triplet and the fundamental parameters of F-G supergiants",Monthly Notices of the Royal Astronomical Society,423 (4):3268–3273,arXiv:1204.4115,Bibcode:2012MNRAS.423.3268K,doi:10.1111/j.1365-2966.2012.21117.x,ISSN 0035-8711,S2CID 118683158.
  7. ^abPasinetti Fracassini, L. E.; et al. (February 2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS)",Astronomy and Astrophysics,367 (2) (Third ed.):521–524,arXiv:astro-ph/0012289,Bibcode:2001A&A...367..521P,doi:10.1051/0004-6361:20000451,S2CID 425754.
  8. ^abHohle, M.M.; et al. (2010), "Masses and luminosities of O- and B-type stars and red supergiants",Astronomische Nachrichten,331 (4): 349,arXiv:1003.2335,Bibcode:2010AN....331..349H,doi:10.1002/asna.200911355,S2CID 111387483.
  9. ^abDanziger, I. J.; Faber, S. M. (May 1972), "Rotation of evolving A and F stars",Astronomy and Astrophysics,18: 428,Bibcode:1972A&A....18..428D.
  10. ^"22 And".SIMBAD.Centre de données astronomiques de Strasbourg. RetrievedSeptember 21, 2018.
  11. ^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.
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