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HD 168592
Location of HD 168592 (circled)
Observation data
Epoch J2000.0       Equinox J2000.0 ( ICRS)
Constellation Corona Australis
Right ascension 18h 22m 18.57340s [1]
Declination −38° 39′ 24.8261″ [1]
Apparent magnitude (V) 5.07±0.01 [2]
Characteristics
Spectral type K4/5 III [3]
B−V color index +1.49 [4]
Astrometry
Radial velocity (Rv)17.8±2.8 [5] km/s
Proper motion (μ) RA: −41.570  mas/ yr [1]
Dec.: −29.379  mas/ yr [1]
Parallax (π)6.7176 ± 0.1706  mas [1]
Distance490 ± 10  ly
(149 ± 4  pc)
Absolute magnitude (MV)−0.76 [6]
Details
Mass1.18 [7]  M☉
Radius43.6±2.2 [8]  R☉
Luminosity666+44
−40 [1]  L☉
Surface gravity (log g)1.34 [7]  cgs
Temperature4,148±122 [9]  K
Metallicity [Fe/H]−0.13±0.01 [10]  dex
Rotational velocity (v sin i)1.9±1.3 [11] km/s
Other designations
7 G. Coronae Australis [12], CD−38°12729, CPD−38°7475, GC 25051, HD 168592, HIP 90037, HR 6862, SAO 210048 [13]
Database references
SIMBAD data

HD 168592, also designated as HR 6862 or rarely 7 G. Coronae Australis, is a solitary star [14] located in the southern constellation Corona Australis. It is faintly visible to the naked eye as an orange-hued star with an apparent magnitude of 5.07. Gaia DR3 parallax measurements place it at a distance of 490 light years [1] and is currently receding with a heliocentric radial velocity of 18  km/s. [5] At its current distance, HD 168592's brightness is diminished by 0.38 magnitudes due to interstellar dust. [15] It has an absolute magnitude of −0.76. [6]

HD 168592 has a stellar classification of K4/5 III, [3] indicating that it is an evolved K-type star with the characteristics of a K4 and K5 giant star. It has a comparable mass to the Sun [7] but the star has expanded to 43.6 times the Sun's radius. [8] It radiates 666 times the luminosity of the Sun [1] from its enlarged photosphere at an effective temperature of 4,148  K. [9] HD 168592 is slightly metal deficient with an iron abundance 26% below solar levels. [10] The star spins slowly, as is common for giant stars, with a projected rotational velocity of 1.9  km/s. [11]

References

  1. ^ a b c d e f g 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.
  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.
  3. ^ a b Houk, N. (1982). Michigan Catalogue of Two-dimensional Spectral Types for the HD stars. Volume III: Declinations −40° to −26°. Bibcode: 1982mcts.book.....H.
  4. ^ Corben, P. M.; Stoy, R. H. (1968). "Photoelectric Magnitudes and Colours for Bright Southern Stars". Monthly Notes of the Astronomical Society of South Africa. 27: 11. Bibcode: 1968MNSSA..27...11C. ISSN  0024-8266.
  5. ^ a b 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.
  6. ^ a b 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. ^ a b c 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.
  8. ^ a b Kervella, P.; Thévenin, F.; Di Folco, E.; Ségransan, D. (October 2004). "The angular sizes of dwarf stars and subgiants". Astronomy & Astrophysics. 426 (1): 297–307. arXiv: astro-ph/0404180. Bibcode: 2004A&A...426..297K. doi: 10.1051/0004-6361:20035930. eISSN  1432-0746. ISSN  0004-6361.
  9. ^ a b 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. hdl: 1721.1/124721. S2CID  166227927.
  10. ^ a b Poggio, E.; Recio-Blanco, A.; Palicio, P. A.; Re Fiorentin, P.; de Laverny, P.; Drimmel, R.; Kordopatis, G.; Lattanzi, M. G.; Schultheis, M.; Spagna, A.; Spitoni, E. (30 September 2022). "The chemical signature of the Galactic spiral arms revealed by Gaia DR3". Astronomy & Astrophysics. 666: L4. arXiv: 2206.14849. Bibcode: 2022A&A...666L...4P. doi: 10.1051/0004-6361/202244361. eISSN  1432-0746. ISSN  0004-6361.
  11. ^ a b 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". Astronomy & Astrophysics. 561: A126. arXiv: 1312.3474. Bibcode: 2014A&A...561A.126D. doi: 10.1051/0004-6361/201220762. eISSN  1432-0746. 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. ^ "HD 168592". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved December 22, 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. S2CID  14878976.
  15. ^ Gontcharov, George A.; Mosenkov, Aleksandr V. (28 September 2017). "Verifying reddening and extinction for Gaia DR1 TGAS main sequence stars". Monthly Notices of the Royal Astronomical Society. 472 (4): 3805–3820. arXiv: 1709.01160. Bibcode: 2017MNRAS.472.3805G. doi: 10.1093/mnras/stx2219. eISSN  1365-2966. ISSN  0035-8711.
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