HD 92589

Last updated • 1 min readFrom Wikipedia, The Free Encyclopedia
HD 92589
Observation data
Epoch J2000.0        Equinox J2000.0 (ICRS)
Constellation Antlia
Right ascension 10h 40m 51.5391s [1]
Declination −35° 44′ 30.176″ [1]
Apparent magnitude  (V)6.39±0.01 [2]
Characteristics
Spectral type G8/K0 III + F/G [3]
U−B color index +0.02 [4]
B−V color index +0.92 [4]
Astrometry
Radial velocity (Rv)11±5.4 [5] km/s
Proper motion (μ)RA: −25.072 mas/yr [1]
Dec.: +5.872 mas/yr [1]
Parallax (π)5.5014±0.1586  mas [1]
Distance 590 ± 20  ly
(182 ± 5  pc)
Absolute magnitude  (MV)−0.78 [6]
Details
A
Mass 2.3 [7]   M☉
Radius 13.07 [8]   R☉
Luminosity 141 [1]   L☉
Surface gravity (log g)2.54 [7]   cgs
Temperature 5,171±122 [9]   K
Metallicity [Fe/H]−0.29 [10]   dex
Rotational velocity (v sin i)1.6±1.2 [11]  km/s
B
Mass 2.96 [12]   M☉
Other designations
76 G. Antliae, CD−35°6646, CPD−35°4320, FK5 2586, HD 92589, HIP 52273, HR 4183, SAO 201631, WDS J10409-3545
Database references
SIMBAD data

HD 92589 (HR 4183) is a double star in the constellation Antlia. The system has a combined apparent magnitude of 6.39, [2] placing it near the limit of naked eye visibility. The system is located about 590  light years [1] away based on its parallax shift and has a heliocentric radial velocity of 11  km/s . [5] This indicates that it is drifting away from the Solar System.

The system has a composite stellar classification of G8/K0 III + F/G. [3] This indicates that the primary spectrum intermediate between a G8 and K0 giant star while the companion is probably a F-type or G-type star. As of 1991, the pair have a projected separation of 700  mas along a position angle of 48° . [13] Both stars take 1,591  years to orbit each other. [13] [12]

At present the visible component has 2.3 times the mass of the Sun [7] but has expanded to 13.07 [8] times its girth. It shines with a luminosity 141 [1] times greater than the Sun from its enlarged photosphere at an effective temperature of 5,171  K , [9] which gives the yellow hue of a G-type star. HD 92589A is metal-deficient, with an iron abundance only 51% [10] that of the Sun and spins leisurely with a projected rotational velocity of 1.6  km/s , [11] common for giant stars.

References

  1. 1 2 3 4 5 6 7 8 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. 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.
  3. 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.
  4. 1 2 Deutschman, W. A.; Davis, R. J.; Schild, R. E. (February 1976). "The galactic distribution of interstellar absorption as determined from the Celescope catalog of ultraviolet stellar observations and a new catalog of UBV, H-beta photoelectric observations". The Astrophysical Journal Supplement Series. 30: 97. Bibcode:1976ApJS...30...97D. doi: 10.1086/190359 . ISSN   0067-0049.
  5. 1 2 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. 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. 1 2 3 Anders, F.; et al. (February 2022). "Photo-astrometric distances, extinctions, and astrophysical parameters for Gaia EDR3 stars brighter than G = 18.5". Astronomy & Astrophysics. 658: A91. arXiv: 2111.01860 . Bibcode:2022A&A...658A..91A. doi: 10.1051/0004-6361/202142369 . eISSN   1432-0746. ISSN   0004-6361.
  8. 1 2 Kervella, Pierre; Arenou, Frédéric; Thévenin, Frédéric (2022). "Stellar and substellar companions from Gaia EDR3". Astronomy & Astrophysics. 657: A7. arXiv: 2109.10912 . Bibcode:2022A&A...657A...7K. doi: 10.1051/0004-6361/202142146 . eISSN   1432-0746. ISSN   0004-6361.
  9. 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 . ISSN   0004-6256.
  10. 1 2 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 . ISSN   0004-6361.
  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. 1 2 Tokovinin, Andrei (23 February 2018). "The Updated Multiple Star Catalog". The Astrophysical Journal Supplement Series. 235 (1): 6. arXiv: 1712.04750 . Bibcode:2018ApJS..235....6T. doi: 10.3847/1538-4365/aaa1a5 . eISSN   1538-4365.
  13. 1 2 Mason, Brian D.; Wycoff, Gary L.; Hartkopf, William I.; Douglass, Geoffrey G.; Worley, Charles E. (December 2001). "The 2001 US Naval Observatory Double Star CD-ROM. I. The Washington Double Star Catalog". The Astronomical Journal. 122 (6): 3466–3471. Bibcode:2001AJ....122.3466M. doi: 10.1086/323920 . ISSN   0004-6256.
This page is based on this Wikipedia article
Text is available under the CC BY-SA 4.0 license; additional terms may apply.
Images, videos and audio are available under their respective licenses.