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HR 2131

From Wikipedia, the free encyclopedia
Star in the constellation Columba
HR 2131
Observation data
EpochJ2000.0      EquinoxJ2000.0 (ICRS)
ConstellationColumba
Right ascension06h 01m 16.298s[1]
Declination−33° 54′ 42.61″[1]
Apparent magnitude (V)5.52±0.01[2]
Characteristics
Spectral typeK5 III[3]
U−Bcolor index+1.94[4]
B−Vcolor index+1.58[4]
Astrometry
Radial velocity (Rv)19.0±7.4[5] km/s
Proper motion (μ)RA: 4.876[1]mas/yr
Dec.: −26.178[1]mas/yr
Parallax (π)4.8320±0.0725 mas[1]
Distance670 ± 10 ly
(207 ± 3 pc)
Absolute magnitude (MV)−0.82[6]
Details
Mass1.81[7] M
Radius49.24[8] R
Luminosity501[7] L
Surface gravity (log g)1.7[9] cgs
Temperature3,700±150[10] K
Metallicity [Fe/H]0.00[10] dex
Rotational velocity (v sin i)2.6±1.1[11] km/s
Age2.19[7] Gyr
Other designations
67 G. Columbae,CD−33°2681,CPD−33°980,GC 7630,HD 41047,HIP 28524,HR 2131,SAO 196413
Database references
SIMBADdata

HR 2131 (HD 41047) is a solitary[12]star in the southern constellationColumba. It has anapparent magnitude of 5.52,[2] allowing it to be faintly seen with thenaked eye. The object is located at a distance of 670light years[1] but is receding with a heliocentricradial velocity of19 km/s.[5]

HR 2131 has astellar classification of K5 III,[3] indicating that it is ared giant. It has 1.81 times themass of the Sun and is 2.19billion years old.[7] The star's high luminosity of501 L[7] and a loweffective temperature of 3,700K[10] causes it to have an enlarged radius 49 times that of theSun.[8] HR 2131'smetallicity – elements heavier thanhelium – is around solar level;[10] it spins with aprojected rotational velocity of about2.6 km/s.[11]

References

[edit]
  1. ^abcdefBrown, 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. ^abHøg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. (March 2000). "The Tycho-2 catalogue of the 2.5 million brightest stars".Astronomy and Astrophysics.355:L27 –L30.Bibcode:2000A&A...355L..27H.ISSN 0004-6361.
  3. ^abHouk, N. (1982).Michigan Catalogue of Two-dimensional Spectral Types for the HD stars. Volume_3. Declinations -40_ƒ0 to -26_ƒ0.Bibcode:1982mcts.book.....H.
  4. ^abMermilliod, J. -C. (1986). "Compilation of Eggen's UBV data, transformed to UBV (unpublished)".Catalogue of Eggen's UBV Data: 0.Bibcode:1986EgUBV........0M.
  5. ^abKharchenko, N.V.; Scholz, R.-D.; Piskunov, A.E.; Röser, S.; Schilbach, E. (November 2007)."Astrophysical supplements to the ASCC-2.5: Ia. Radial velocities of ~55000 stars and mean radial velocities of 516 Galactic open clusters and associations".Astronomische Nachrichten.328 (9):889–896.arXiv:0705.0878.Bibcode:2007AN....328..889K.doi:10.1002/asna.200710776.ISSN 0004-6337.
  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.ISSN 1063-7737.S2CID 255204555.
  7. ^abcdeLuck, R. Earle (September 2015)."Abundances in the Local Region. I. G and K Giants".The Astronomical Journal.150 (3): 88.arXiv:1507.01466.Bibcode:2015AJ....150...88L.doi:10.1088/0004-6256/150/3/88.ISSN 0004-6256.
  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. ^Lafrasse, Sylvain; Mella, Guillaume; Bonneau, Daniel; Duvert, Gilles; Delfosse, Xavier; Chesneau, Olivier; Chelli, Alain (16 July 2010). "Building the 'JMMC Stellar Diameters Catalog' using SearchCal".Optical and Infrared Interferometry II. Vol. 7734. pp. 77344E.arXiv:1009.0137.Bibcode:2010SPIE.7734E..4EL.doi:10.1117/12.857024.S2CID 32097037.
  10. ^abcdCharbonnel, C.; Lagarde, N.; Jasniewicz, G.; North, P. L.; Shetrone, M.; Krugler Hollek, J.; Smith, V. V.; Smiljanic, R.; Palacios, A.; Ottoni, G. (January 2020)."Lithium in red giant stars: Constraining non-standard mixing with large surveys in the Gaia era".Astronomy & Astrophysics.633: A34.arXiv:1910.12732.Bibcode:2020A&A...633A..34C.doi:10.1051/0004-6361/201936360.ISSN 0004-6361.
  11. ^abDe Medeiros, J. R.; Alves, S.; Udry, S.; Andersen, J.; Nordström, B.; Mayor, M. (January 2014)."A catalog of rotational and radial velocities for evolved stars: V. Southern stars⋆⋆⋆".Astronomy & Astrophysics.561: A126.arXiv:1312.3474.Bibcode:2014A&A...561A.126D.doi:10.1051/0004-6361/201220762.ISSN 0004-6361.
  12. ^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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