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Omega Hydrae

From Wikipedia, the free encyclopedia
Star in the constellation Hydra
Omega Hydrae
Location of ω Hydrae (circled in red)
Observation data
EpochJ2000.0      EquinoxJ2000.0 (ICRS)
ConstellationHydra
Right ascension09h 05m 58.36642s[1]
Declination+05° 05′ 32.3360″[1]
Apparent magnitude (V)5.00[2]
Characteristics
Evolutionary stagehorizontal branch[3]
Spectral typeK2 II-III[4]
U−Bcolor index+1.22[2]
B−Vcolor index+1.22[2]
Astrometry
Radial velocity (Rv)+24.3±0.8[5] km/s
Proper motion (μ)RA: −19.58[1]mas/yr
Dec.: −11.07[1]mas/yr
Parallax (π)3.64±0.31 mas[1]
Distance900 ± 80 ly
(270 ± 20 pc)
Absolute magnitude (MV)−2.19[6]
Details[3]
Mass4.32±0.37 M
Radius48.49±5.55 R
Luminosity944.3±178.3 L
Surface gravity (log g)1.74±0.12 cgs
Temperature4,789[7] K
Metallicity[Fe/H]−0.12±0.10 dex
Rotational velocity (v sin i)2.3[8] km/s
Age180±70 Myr
Other designations
ω Hya,18 Hydrae,BD+05°2116,HD 77996,HIP 44659,HR 3613,SAO 117420[9]
Database references
SIMBADdata

Omega Hydrae,Latinised fromω Hydrae, is a golden-huedstar in theequatorialconstellation ofHydra, located to the west-southwest of the brighter starZeta Hydrae.[10] Based upon an annualparallax shift of just 3.64 mas as seen from Earth, it is located roughly 900 light-years from theSun. It is faintly visible to the naked eye with anapparent visual magnitude of 5.00.[2]

This is anevolvedK-type star with astellar classification of K2 II-III,[4] which indicates aspectrum showing traits intermediate between thegiant andbright giant stages. It is most likely (98% chance) on thehorizontal branch, indicating that the star is generating energy through thethermonuclear fusion of helium at its core. With 4.32 times theSun's mass, it has expanded to around 48 times theradius of the Sun. Omega Hydrae is about 180[3] million years old and spinning with a leisurelyprojected rotational velocity of 2.3 km/s.[8] The star is radiating roughly 944[3] times thesolar luminosity from itsphotosphere at aneffective temperature of4,789 K.[7]

References

[edit]
  1. ^abcdevan Leeuwen, F. (2007), "Validation of the new Hipparcos reduction",Astronomy and Astrophysics,474 (2):653–664,arXiv:0708.1752,Bibcode:2007A&A...474..653V,doi:10.1051/0004-6361:20078357,S2CID 18759600.
  2. ^abcdMermilliod, J.-C. (1986), "Compilation of Eggen's UBV data, transformed to UBV (unpublished)",Catalogue of Eggen's UBV Data,SIMBAD,Bibcode:1986EgUBV........0M.
  3. ^abcdReffert, Sabine; et al. (2015), "Precise radial velocities of giant stars. VII. Occurrence rate of giant extrasolar planets as a function of mass and metallicity",Astronomy & Astrophysics,574: A116,arXiv:1412.4634,Bibcode:2015A&A...574A.116R,doi:10.1051/0004-6361/201322360,hdl:10722/215277,S2CID 59334290.Values are for the higher probability horizontal branch model fit.
  4. ^abTetzlaff, N.; et al. (2011)."A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun".Monthly Notices of the Royal Astronomical Society.410 (1):190–200.arXiv:1007.4883.Bibcode:2011MNRAS.410..190T.doi:10.1111/j.1365-2966.2010.17434.x.S2CID 118629873.
  5. ^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,arXiv:1208.3048,Bibcode:2012A&A...546A..61D,doi:10.1051/0004-6361/201219219,S2CID 59451347, A61.
  6. ^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.
  7. ^abMcDonald, I.; et al. (2012), "Fundamental Parameters and Infrared Excesses of Hipparcos Stars",Monthly Notices of the Royal Astronomical Society,427 (1):343–57,arXiv:1208.2037,Bibcode:2012MNRAS.427..343M,doi:10.1111/j.1365-2966.2012.21873.x,S2CID 118665352.
  8. ^abLèbre, A.; et al. (May 2006), "Lithium abundances and rotational behavior for bright giant stars",Astronomy and Astrophysics,450 (3):1173–1179,Bibcode:2006A&A...450.1173L,doi:10.1051/0004-6361:20053485
  9. ^"* ome Hya".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2017-03-17.{{cite web}}: CS1 maint: postscript (link)
  10. ^O'Meara, Stephen James (2016),Deep-Sky Companions: The Caldwell Objects,Cambridge University Press, p. 224,ISBN 978-1107083974

External links

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