12 Hydrae
Observation data
Epoch J2000      Equinox J2000
Constellation Hydra
Right ascension 08h 46m 22.53544s[1]
Declination −13° 32′ 51.7502″[1]
Apparent magnitude (V) 4.32[2]
Characteristics
Spectral type G8 IIIb CN-1[3]
B−V color index 0.900±0.015[2]
Astrometry
Radial velocity (Rv)−8.5±0.7[2] km/s
Proper motion (μ) RA: +18.789[1] mas/yr
Dec.: −18.385[1] mas/yr
Parallax (π)16.1839 ± 0.6646 mas[1]
Distance202 ± 8 ly
(62 ± 3 pc)
Absolute magnitude (MV)+0.26[4]
Orbit[5]
PrimaryAa
CompanionAb
Period (P)1,592±806 d
Semi-major axis (a)0.0116±0.057″
Eccentricity (e)0.40±0.26
Inclination (i)58±10°
Longitude of the node (Ω)91±16°
Periastron epoch (T)49,194±664
Argument of periastron (ω)
(secondary)		103±34°
Details
Mass2.32[6] M☉
Radius11.51+0.18
−0.37[1] R☉
Luminosity77.468±3.553[1] L☉
Temperature4,968±13[6] K
Rotational velocity (v sin i)4.6±0.2[4] km/s
Age910[6] Myr
Other designations
D Hya, 12 Hya, BD−13°2673, HD 74918, HIP 43067, HR 3484, SAO 154622, WDS J08464-1333[7]
Database references
SIMBADdata

12 Hydrae is a probable astrometric binary[8] star system located 202 light years away from the Sun in the equatorial constellation of Hydra. It has the Bayer designation D Hydrae;[7] 12 Hydrae is the Flamsteed designation. This system is visible to the naked eye as a faint, yellow-hued star with a combined apparent visual magnitude of 4.32.[2] It is moving closer to the Earth with a heliocentric radial velocity of −8.5 km/s.[2]

This was found to be a double star by R. A. Rossiter in 1953,[9] with the magnitude 13.7 companion having an angular separation of 26.8″ along a position angle of 266°, as of 2016. The brighter, magnitude 4.32 component A is a spectroscopic binary. As of 2009, the orbital solution for this pair is of low quality, giving a period of roughly 4 years and an eccentricity of around 0.4.[5]

The primary component is an aging giant star with a stellar classification of G8 IIIb CN-1,[3] where the suffix notation indicates an underabundance of the cyanogen molecule. It is 910[6] million years old with 2.32[6] times the mass of the Sun. After exhausting the hydrogen at its core and evolving off the main sequence, the star has swollen to 11.5[1] times the Sun's radius. It is radiating 77[1] times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 4,968 K.[6]

References

  1. ^ a b c d e f g h i Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
  2. ^ a b c d e 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, S2CID 119257644.
  3. ^ a b Keenan, Philip C.; McNeil, Raymond C. (1989), "The Perkins catalog of revised MK types for the cooler stars", Astrophysical Journal Supplement Series, 71: 245, Bibcode:1989ApJS...71..245K, doi:10.1086/191373
  4. ^ a b Ammler-von Eiff, Matthias; Reiners, Ansgar (June 2012), "New measurements of rotation and differential rotation in A-F stars: are there two populations of differentially rotating stars?", Astronomy & Astrophysics, 542: A116, arXiv:1204.2459, Bibcode:2012A&A...542A.116A, doi:10.1051/0004-6361/201118724, S2CID 53666672.
  5. ^ a b Hartkopf, W. I.; et al. (June 30, 2006), Sixth Catalog of Orbits of Visual Binary Stars, United States Naval Observatory, archived from the original on 2017-08-01, retrieved 2017-06-02.
  6. ^ a b c d e f Luck, R. Earle (2015), "Abundances in the Local Region. I. G and K Giants", Astronomical Journal, 150 (3), 88, arXiv:1507.01466, Bibcode:2015AJ....150...88L, doi:10.1088/0004-6256/150/3/88, S2CID 118505114.
  7. ^ a b "12 Hya". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved May 1, 2019.
  8. ^ 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, arXiv:0806.2878, Bibcode:2008MNRAS.389..869E, doi:10.1111/j.1365-2966.2008.13596.x, S2CID 14878976.
  9. ^ Rossiter, R. A. (February 1953), "Seventh list of new Southern double stars found at the Lamont-Hussey Observatory of the University of Michigan at Bloemfontein, South Africa.", Astronomical Journal, 58: 29–30, Bibcode:1953AJ.....58...29R, doi:10.1086/106804.
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