Astronomy:HR 2131
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Short description: Star in the constellation Columba
| Observation data Epoch J2000.0 Equinox (celestial coordinates) | |
|---|---|
| Constellation | Columba |
| Right ascension | 06h 01m 16.298s[1] |
| Declination | −33° 54′ 42.61″[1] |
| Apparent magnitude (V) | 5.52±0.01[2] |
| Characteristics | |
| Spectral type | K5 III[3] |
| U−B color index | +1.94[4] |
| B−V color 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[1] mas |
| Distance | 670 ± 10 ly (207 ± 3 pc) |
| Absolute magnitude (MV) | −0.82[6] |
| Details | |
| Mass | 1.81[7] M☉ |
| Radius | 49.24[8] R☉ |
| Luminosity | 501[7] L☉ |
| Surface gravity (log g) | 1.7[9] cgs |
| Temperature | 3,700±150[10] K |
| Metallicity [Fe/H] | 0.00[10] dex |
| Rotational velocity (v sin i) | 2.6±1.1[11] km/s |
| Age | 2.19[7] Gyr |
| Other designations | |
| Database references | |
| SIMBAD | data |
HR 2131 (HD 41047) is a solitary[12] star in the southern constellation Columba. It has an apparent magnitude of 5.52,[2] allowing it to be faintly seen with the naked eye. The object is located at a distance of 670 light years[1] but is receding with a heliocentric radial velocity of 19 km/s.[5]
HR 2131 has a stellar classification of K5 III,[3] indicating that it is a red giant. It has 1.81 times the mass of the Sun and is 2.19 billion years old.[7] The star's high luminosity of 501 solar luminosity[7] and a low effective temperature of 3,700 K[10] causes it to have an enlarged radius 49 times that of the Sun.[8] HR 2131's metallicity – elements heavier than helium – is around solar level;[10] it spins with a projected rotational velocity of about 2.6 km/s.[11]
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 Brown, A. G. A. (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics 649: A1. doi:10.1051/0004-6361/202039657. Bibcode: 2021A&A...649A...1G. Gaia EDR3 record for this source at VizieR.
- ↑ 2.0 2.1 Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P. et al. (March 2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics 355: L27–L30. ISSN 0004-6361. Bibcode: 2000A&A...355L..27H.
- ↑ 3.0 3.1 Houk, 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.
- ↑ 4.0 4.1 Mermilliod, J. -C. (1986). "Compilation of Eggen's UBV data, transformed to UBV (unpublished)". Catalogue of Eggen's UBV Data: 0. Bibcode: 1986EgUBV........0M.
- ↑ 5.0 5.1 Kharchenko, 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. doi:10.1002/asna.200710776. ISSN 0004-6337. Bibcode: 2007AN....328..889K.
- ↑ Anderson, E.; Francis, Ch. (May 2012). "XHIP: An extended hipparcos compilation" (in en). Astronomy Letters 38 (5): 331–346. doi:10.1134/S1063773712050015. ISSN 1063-7737. Bibcode: 2012AstL...38..331A.
- ↑ 7.0 7.1 7.2 7.3 7.4 Luck, R. Earle (September 2015). "Abundances in the Local Region. I. G and K Giants". The Astronomical Journal 150 (3): 88. doi:10.1088/0004-6256/150/3/88. ISSN 0004-6256. Bibcode: 2015AJ....150...88L.
- ↑ 8.0 8.1 Stassun, Keivan G. et al. (9 September 2019). "The Revised TESS Input Catalog and Candidate Target List". The Astronomical Journal 158 (4): 138. doi:10.3847/1538-3881/ab3467. ISSN 0004-6256. Bibcode: 2019AJ....158..138S.
- ↑ 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. 7734. pp. 77344E. doi:10.1117/12.857024. Bibcode: 2010SPIE.7734E..4EL.
- ↑ 10.0 10.1 10.2 10.3 Charbonnel, C.; Lagarde, N.; Jasniewicz, G.; North, P. L.; Shetrone, M.; Krugler Hollek, J.; Smith, V. V.; Smiljanic, R. et al. (January 2020). "Lithium in red giant stars: Constraining non-standard mixing with large surveys in the Gaia era". Astronomy & Astrophysics 633: A34. doi:10.1051/0004-6361/201936360. ISSN 0004-6361. Bibcode: 2020A&A...633A..34C.
- ↑ 11.0 11.1 De 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. doi:10.1051/0004-6361/201220762. ISSN 0004-6361. Bibcode: 2014A&A...561A.126D.
- ↑ 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. doi:10.1111/j.1365-2966.2008.13596.x. Bibcode: 2008MNRAS.389..869E.
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