HD 86267

Last updated
HD 86267
Observation data
Epoch J2000.0        Equinox J2000.0 (ICRS)
Constellation Antlia [1]
Right ascension 09h 56m 35.4937s [2]
Declination −33° 25′ 06.587″ [2]
Apparent magnitude  (V)5.82±0.01 [3]
Characteristics
Evolutionary stage RGB [2]
Spectral type K1 III [4]
B−V color index +1.2 [5]
Astrometry
Radial velocity (Rv)3.7±0.4 [6] km/s
Proper motion (μ)RA: +34.064 mas/yr [2]
Dec.: +22.102 mas/yr [2]
Parallax (π)6.3494±0.0453  mas [2]
Distance 514 ± 4  ly
(157 ± 1  pc)
Absolute magnitude  (MV)−0.15 [1]
Details
Mass 1.73+1.24
−0.71 [7]   M☉
Radius 19.7 [8]   R☉
Luminosity 158±11 [7]   L☉
Surface gravity (log g)1.86 [9]   cgs
Temperature 4430±110 [7]   K
Metallicity [Fe/H]−0.15 [10]   dex
Rotational velocity (v sin i)<1 [11]  km/s
Other designations
36 G. Antliae [12] , CD−32°6895, CPD−32°2771, FK5 2796, GC 13695, HD 86267, HIP 48748, HR 3932, SAO 200889 [13]
Database references
SIMBAD data

HD 86267, also known as HR 3932, is a solitary [14] orange-hued star located in the southern constellation Antlia. It has an apparent magnitude of 5.82, [3] allowing it to be faintly seen with the naked eye. Parallax measurements place it a distance of 514 light years [2] and it is currently receding with a heliocentric radial velocity of 3.7  km/s . [6]

HD 86267 has a stellar classification of K1 III, [4] indicating that it is a red giant. At present it has 1.73 times the mass of the Sun [7] but has expanded to 19.7 times its girth. [8] It shines with a luminosity of 158  L☉ from its enlarged photosphere at an effective temperature of 4,430  K . [7] It is a member of the old disk population, having a metallicity 71% that of the Sun. [10] The value means that it is metal deficient. Its current rotation rate is too low to be measured accurately. [11]

References

  1. 1 2 Anderson, 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. XHIP record for this object at VizieR.
  2. 1 2 3 4 5 6 7 Vallenari, 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 at VizieR.
  3. 1 2 Høg, 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.
  4. 1 2 Houk, N. (1982). Michigan Catalogue of Two-dimensional Spectral Types for the HD stars. Volume_3. Declinations −40° to −26°. Bibcode:1982mcts.book.....H.
  5. ↑ Johnson, H. L.; Mitchell, R. I.; Iriarte, B.; Wisniewski, W. Z. (1966). "UBVRIJKL Photometry of the Bright Stars". Communications of the Lunar and Planetary Laboratory. 4: 99–110. Bibcode:1966CoLPL...4...99J.
  6. 1 2 Gontcharov, 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.
  7. 1 2 3 4 5 Charbonnel, 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 . eISSN   1432-0746. ISSN   0004-6361.
  8. 1 2 Stassun, 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 . eISSN   1538-3881.
  9. ↑ Anders, F.; et al. (August 2019). "Photo-astrometric distances, extinctions, and astrophysical parameters for Gaia DR2 stars brighter than G = 18". Astronomy & Astrophysics. 628: A94. arXiv: 1904.11302 . Bibcode:2019A&A...628A..94A. doi: 10.1051/0004-6361/201935765 . eISSN   1432-0746. ISSN   0004-6361.
  10. 1 2 Eggen, Olin J. (April 1989). "Large and kinematically unbiased samples of G- and K-type stars. IV - Evolved stars of the old disk population". Publications of the Astronomical Society of the Pacific. 101: 366. Bibcode:1989PASP..101..366E. doi: 10.1086/132442 . eISSN   1538-3873. ISSN   0004-6280.
  11. 1 2 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. arXiv: 1312.3474 . Bibcode:2014A&A...561A.126D. doi: 10.1051/0004-6361/201220762 . ISSN   0004-6361.
  12. ↑ Gould, Benjamin Apthorp (1878). "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.
  13. ↑ "HR 3932". SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 4 August 2022.
  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.
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