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HD 85951

From Wikipedia, the free encyclopedia
Star in the constellation of Hydra
HD 85951
Observation data
EpochJ2000.0      EquinoxJ2000.0
ConstellationHydra
Right ascension09h 54m 52.2045s[1]
Declination−19° 00′ 33.620″[1]
Apparent magnitude (V)4.94[2]
Characteristics
Evolutionary stageAGB[3]
Spectral typeK5 III[4]
U−Bcolor index+1.93[2]
B−Vcolor index+1.57[2]
Astrometry
Radial velocity (Rv)50±4.2[5] km/s
Proper motion (μ)RA: −45.386mas/yr[1]
Dec.: −40.456mas/yr[1]
Parallax (π)5.6789±0.2214 mas[1]
Distance570 ± 20 ly
(176 ± 7 pc)
Absolute magnitude (MV)−1.43[6]
Details
Mass6.40+1.2
−0.4
[7] M
Radius56.7[8] R
Luminosity721±32[9] L
Surface gravity (log g)1.3±0.04[10] cgs
Temperature3,875±39[10] K
Metallicity [Fe/H]−0.18±0.07[10] dex
Other designations
Felis,183 G. Hydrae[11],BD−18° 2810,FK5 373,GC 13644,HIP 48615,HR 3923,SAO 155588[12]
Database references
SIMBADdata

HD 85951 (HR 3923), formally namedFelis/ˈflɪs/,[13] is a solitary[14] orange huedstar in theconstellationHydra. It has anapparent magnitude of 4.94,[2] making it faintly visible to thenaked eye under ideal conditions. Based onparallax measurements, the object is about 570light-years away from theSun[1] and is receding with a heliocentricradial velocity of50 km/s.[5]

Nomenclature

[edit]

HD 85951 was the brightest star in the now-obsoleteconstellation ofFelis.[15] In 2016, the IAU organized aWorking Group on Star Names (WGSN)[16] to catalog and standardize proper names for stars. The WGSN approved the nameFelis for this star on 1 June 2018 and it is now so included in the List of IAU-approved Star Names.[13]

Properties

[edit]

This an evolvedred giant with astellar classification of K5 III.[4] It is currently on theasymptotic giant branch,[3] generating energy via fusion ofhydrogen andhelium shells around an inertcarboncore. At present Felis has 6.4 times themass of the Sun[7] and due to its evolved status, has an enlargedradius of56.7 R.[8] It radiates at abolometric luminosity 721 times that of theSun[9] from itsphotosphere at an effective temperature of3,875 K.[10] Felis has aniron abundance 66% that of the Sun, making it metal deficient.

References

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  1. ^abcdeBrown, A. G. A.; et al. (Gaia collaboration) (2021)."Gaia Early Data Release 3: Summary of the contents and survey properties".Astronomy & Astrophysics.649: A1.arXiv:2012.01533.Bibcode:2021A&A...649A...1G.doi:10.1051/0004-6361/202039657.S2CID 227254300. (Erratum: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source atVizieR.
  2. ^abcdDucati, J. R. (2002). "VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system".CDS/ADC Collection of Electronic Catalogues.2237.Bibcode:2002yCat.2237....0D.
  3. ^abEggen, Olin J. (July 1992)."Asymptotic giant branch stars near the sun".The Astronomical Journal.104: 275.Bibcode:1992AJ....104..275E.doi:10.1086/116239.ISSN 0004-6256.
  4. ^abHouk, N.; Smith-Moore, M. (1988).Michigan Catalogue of Two-dimensional Spectral Types for the HD Stars. Volume 4, Declinations -26° to -12°. Vol. 4.Bibcode:1988mcts.book.....H.
  5. ^abGontcharov, G. A. (November 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.eISSN 1562-6873.ISSN 1063-7737.S2CID 119231169.
  6. ^Anderson, E.; Francis, Ch. (May 2012). "XHIP: An extended hipparcos compilation".Astronomy Letters.38 (5):331–346.arXiv:1108.4971.Bibcode:2012AstL...38..331A.doi:10.1134/S1063773712050015.eISSN 1562-6873.ISSN 1063-7737.S2CID 119257644.
  7. ^abVallenari, 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.
  8. ^abStassun, Keivan G.; et al. (9 September 2019)."The Revised TESS Input Catalog and Candidate Target List".The Astronomical Journal.158 (4): 138.arXiv:1905.10694.Bibcode:2019AJ....158..138S.doi:10.3847/1538-3881/ab3467.ISSN 0004-6256.
  9. ^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.
  10. ^abcdArentsen, Anke; Prugniel, Philippe; Gonneau, Anais; Lançon, Ariane; Trager, Scott; Peletier, Reynier; Lyubenova, Mariya; Chen, Yan-Ping; Falcón Barroso, Jesús; Sánchez Blázquez, Patricia; Vazdekis, Alejandro (July 2019)."Stellar atmospheric parameters for 754 spectra from the X-shooter Spectral Library".Astronomy & Astrophysics.627: A138.arXiv:1907.06391.Bibcode:2019A&A...627A.138A.doi:10.1051/0004-6361/201834273.eISSN 1432-0746.ISSN 0004-6361.
  11. ^Gould, Benjamin Apthorp (January 1879). "Uranometria Argentina : brillantez y posicion de las estrellas fijas, hasta la septima magnitud, comprendidas dentro de cien grados del polo austral : con atlas".Resultados del Observatorio Nacional Argentino.1.Bibcode:1879RNAO....1.....G.
  12. ^"HD 85951".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved30 September 2012.
  13. ^ab"Naming Stars". IAU.org. Retrieved18 June 2018.
  14. ^Eggleton, P. P.; Tokovinin, A. A. (11 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.eISSN 1365-2966.ISSN 0035-8711.
  15. ^"Star Tales Felis". Retrieved16 January 2021.
  16. ^"IAU Working Group on Star Names (WGSN)". Retrieved22 May 2016.
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