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2 Pegasi

From Wikipedia, the free encyclopedia
Star in the constellation Pegasus
2 Pegasi
Location of 2 Pegasi (circled)
Observation data
Epoch J2000      Equinox J2000
ConstellationPegasus
Right ascension21h 29m 56.89545s[1]
Declination23° 38′ 19.8170″[1]
Apparent magnitude (V)4.52[2]
Characteristics
Evolutionary stageAGB[3]
Spectral typeM1+III[4]
U−Bcolor index+1.93[5]
B−Vcolor index+1.62[5]
Astrometry
Radial velocity (Rv)−18.92[6] km/s
Proper motion (μ)RA: +24.74[1]mas/yr
Dec.: +3.63[1]mas/yr
Parallax (π)8.28±0.18 mas[1]
Distance394 ± 9 ly
(121 ± 3 pc)
Absolute magnitude (MV)−0.89[2]
Details
Mass1.2[7] M
Radius55[8] R
Luminosity646[9] L
Surface gravity (log g)1.57[7] cgs
Temperature3,921[9] K
Metallicity[Fe/H]−0.16[7] dex
Other designations
2 Peg,NSV 25624,BD+23°4325,FK5 1565,GC 30109,HD 204724,HIP 106140,HR 8225,SAO 89752,CCDM J21299+2338A,WDS J21299+2338A[10]
Database references
SIMBADdata

2 Pegasi is a single[11]star in theconstellationPegasus, located approximately 394 light years away from the Sun based on parallax.[1] It is visible to thenaked eye as a faint, red-hued star with anapparent visual magnitude of 4.52.[2] The object is moving closer to the Earth with a heliocentricradial velocity of −19 km/s.[6] It has a magnitude 12.7 visual companion, designated component B, at anangular separation of30.4.[12]

This is an agingred giant star with astellar classification of M1+III,[4] currently on theasymptotic giant branch,[3] having exhausted the hydrogen at its core andevolved away from themain sequence. The star has expanded to an estimated 55 times theradius of the Sun.[8] It is radiating 646 times theluminosity of the Sun from its enlargedphotosphere at aneffective temperature of3,921 K.

It is the 2nd star numbered byFlamsteed in order ofright ascension. In the 1795 French-language Fortin-Flamsteed edition of theAtlas Coelestis, 2 Pegasi is labelled with the letter "f".[13]

References

[edit]
  1. ^abcdefVan Leeuwen, F. (2007). "Validation of the new Hipparcos reduction".Astronomy and Astrophysics.474 (2):653–664.arXiv:0708.1752.Bibcode:2007A&A...474..653V.doi:10.1051/0004-6361:20078357.S2CID 18759600.Vizier catalog entry
  2. ^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.Vizier catalog entry
  3. ^abEggen, O. J. (1992). "Asymptotic giant branch stars near the sun".The Astronomical Journal.104: 275.Bibcode:1992AJ....104..275E.doi:10.1086/116239.
  4. ^abHoffleit, D.; Warren, W. H. (1995). "VizieR Online Data Catalog: Bright Star Catalogue, 5th Revised Ed. (Hoffleit+, 1991)".VizieR On-line Data Catalog: V/50. Originally Published in: 1964BS....C......0H.5050.Bibcode:1995yCat.5050....0H.
  5. ^abMallama, A. (2014). "Sloan Magnitudes for the Brightest Stars".The Journal of the American Association of Variable Star Observers.42 (2): 443.Bibcode:2014JAVSO..42..443M.Vizier catalog entry
  6. ^abFamaey, B.; Pourbaix, D.; Frankowski, A.; Van Eck, S.; Mayor, M.; Udry, S.; Jorissen, A. (2009). "Spectroscopic binaries among Hipparcos M giants".Astronomy and Astrophysics.498 (2): 627.arXiv:0901.0934.Bibcode:2009A&A...498..627F.doi:10.1051/0004-6361/200810698.S2CID 18739721.
  7. ^abcKhalatyan, A.; Anders, F.; Chiappini, C.; Queiroz, A. B. A.; Nepal, S.; Dal Ponte, M.; Jordi, C.; Guiglion, G.; Valentini, M.; Torralba Elipe, G.; Steinmetz, M.; Pantaleoni-González, M.; Malhotra, S.; Jiménez-Arranz, Ó.; Enke, H.; Casamiquela, L.; Ardèvol, J. (2024). "Transferring spectroscopic stellar labels to 217 million Gaia DR3 XP stars with SHBoost".Astronomy and Astrophysics.691: A98.arXiv:2407.06963.Bibcode:2024A&A...691A..98K.doi:10.1051/0004-6361/202451427.
  8. ^abBrown, 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. Gaia DR2 record for this source atVizieR.
  9. ^abLehtinen, Jyri J.; Spada, Federico; Käpylä, Maarit J.; Olspert, Nigul; Käpylä, Petri J. (2020). "Common dynamo scaling in slowly rotating young and evolved stars".Nature Astronomy.4 (7): 658.arXiv:2003.08997.Bibcode:2020NatAs...4..658L.doi:10.1038/s41550-020-1039-x.
  10. ^"2 Peg".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2019-04-07.
  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.
  12. ^Mason, Brian D.; Wycoff, Gary L.; Hartkopf, William I.; Douglass, Geoffrey G.; Worley, Charles E. (2001)."The 2001 US Naval Observatory Double Star CD-ROM. I. The Washington Double Star Catalog".The Astronomical Journal.122 (6): 3466.Bibcode:2001AJ....122.3466M.doi:10.1086/323920.Vizier catalog entry
  13. ^Flamsteed, John; Fortin, Jean Nicolas; De Lalande, Joseph Jerome Lefrancais (1795). "Atlas celeste".Paris: Delamarche.Bibcode:1795atce.book.....F.
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