Astronomy:HD 24160

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Short description: Star in the constellation Eridanus
HD 24160
Location of HD 24160 (circled)
Observation data
Equinox J2000.0]] (ICRS)
Constellation Eridanus[1]
Right ascension  03h 49m 27.24527s[2]
Declination −36° 12′ 34.8771″[2]
Apparent magnitude (V) 4.17[1]
Characteristics
Evolutionary stage red clump[3]
Spectral type G7 III[4]
B−V color index 0.927±0.045[1]
Astrometry
Radial velocity (Rv)+2.0±0.7[5] km/s
Proper motion (μ) RA: −45.547(77)[2] mas/yr
Dec.: −49.503(108)[2] mas/yr
Parallax (π)14.9781 ± 0.0915[2] mas
Distance218 ± 1 ly
(66.8 ± 0.4 pc)
Absolute magnitude (MV)0.13[1]
Details
Mass2.33[6] M☉
Radius11[7] R☉
Luminosity81.3[6] L☉
Surface gravity (log g)2.85±0.08[8] cgs
Temperature4,948±45[6] K
Metallicity [Fe/H]+0.08±0.02[8] dex
Age1.76[6] Gyr
Other designations
g Eri, CD−36°1467, FK5 143, HD 24160, HIP 17874, HR 1195, SAO 194559[9]
Database references
SIMBADdata

HD 24160 is a single[10] star in the equatorial constellation of Eridanus. It has the Bayer designation g Eridani. It is visible to the naked eye with an apparent visual magnitude of 4.17.[1] The distance to HD 24160 can be estimated from its annual parallax shift of 14.98 mas,[2] yielding a separation of 218 light years. It is moving further from the Earth with a heliocentric radial velocity of +2 km/s.[5] This object is a coronal member of the Ursa Major Moving Group of stars that share a common motion through space.[11]

At the age of 1.76 billion years old, HD 24160 is an evolved G-type giant star with a stellar classification of G7 III,[4] having consumed the hydrogen at its core and tracked away from the main sequence. It has 2.33[6] times the mass of the Sun and has expanded to about 11[7] times the Sun's radius. The star is radiating 81.3[6] times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,948 K.[6]

References

  1. ↑ 1.0 1.1 1.2 1.3 1.4 Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters 38 (5): 331. doi:10.1134/S1063773712050015. Bibcode: 2012AstL...38..331A  XHIP record for this object at VizieR.
  2. ↑ 2.0 2.1 2.2 2.3 2.4 Vallenari, A. et al. (2022). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy & Astrophysics. doi:10.1051/0004-6361/202243940  Gaia DR3 record for this source at VizieR.
  3. ↑ Gontcharov, G. A. (2008). "Red giant clump in the Tycho-2 catalogue". Astronomy Letters 34 (11): 785–796. doi:10.1134/S1063773708110078. Bibcode: 2008AstL...34..785G. 
  4. ↑ 4.0 4.1 Keenan, Philip C.; McNeil, Raymond C. (1989), "The Perkins catalog of revised MK types for the cooler stars", Astrophysical Journal Supplement Series 71: 245, doi:10.1086/191373, Bibcode: 1989ApJS...71..245K. 
  5. ↑ 5.0 5.1 de Bruijne, J. H. J.; Eilers, A.-C. (October 2012), "Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project", Astronomy & Astrophysics 546: 14, doi:10.1051/0004-6361/201219219, A61, Bibcode: 2012A&A...546A..61D. 
  6. ↑ 6.0 6.1 6.2 6.3 6.4 6.5 6.6 Luck, R. Earle (2015), "Abundances in the Local Region. I. G and K Giants", Astronomical Journal 150 (3), doi:10.1088/0004-6256/150/3/88, Bibcode: 2015AJ....150...88L. 
  7. ↑ 7.0 7.1 Pasinetti Fracassini, L. E. et al. (February 2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS) - Third edition - Comments and statistics", Astronomy and Astrophysics 367 (2): 521–524, doi:10.1051/0004-6361:20000451, Bibcode: 2001A&A...367..521P. 
  8. ↑ 8.0 8.1 Alves, S. et al. (April 2015), "Determination of the spectroscopic stellar parameters for 257 field giant stars", Monthly Notices of the Royal Astronomical Society 448 (3): 2749–2765, doi:10.1093/mnras/stv189, Bibcode: 2015MNRAS.448.2749A. 
  9. ↑ "HD 24160". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=HD+24160. 
  10. ↑ Eggleton, P. P.; Tokovinin, A. A. (2008), "A catalogue of multiplicity among bright stellar systems", Monthly Notices of the Royal Astronomical Society 389 (2): 869, doi:10.1111/j.1365-2966.2008.13596.x, Bibcode: 2008MNRAS.389..869E. 
  11. ↑ Chupina, N. V. et al. (June 2006), "Kinematic structure of the corona of the Ursa Major flow found using proper motions and radial velocities of single stars", Astronomy and Astrophysics 451 (3): 909–916, doi:10.1051/0004-6361:20054009, Bibcode: 2006A&A...451..909C.