Astronomy:Xi Hydrae

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Short description: Star in the constellation Hydra
Xi Hydrae
Observation data
Equinox J2000.0]] (ICRS)
Constellation Hydra
Right ascension  11h 33m 00.11505s[1]
Declination −31° 51′ 27.4435″[1]
Apparent magnitude (V) 3.54[2]
Characteristics
Spectral type G7 III[2]
Astrometry
Radial velocity (Rv)−4.90±0.30[3] km/s
Proper motion (μ) RA: −209.62[1] mas/yr
Dec.: −40.84[1] mas/yr
Parallax (π)25.16 ± 0.16[1] mas
Distance129.6 ± 0.8 ly
(39.7 ± 0.3 pc)
Absolute magnitude (MV)+0.54[4]
Details
Mass2.94±0.15[5] M
Radius10.2±0.1[6] R
Luminosity57.65±2.39[6] L
Surface gravity (log g)2.87±0.02[5] cgs
Temperature5,044±40[5] K
Metallicity [Fe/H]+0.16±0.20[5] dex
Rotational velocity (v sin i)2.7[6] km/s
Other designations
ξ Lyr, 288 G. Hydrae,[7] CD−31° 9083, HD 100407, HIP 56343, HR 4450, SAO 202558[8]
Database references
SIMBADdata
One possible non-radial oscillation mode of Xi Hydrae

Xi Hydrae, Latinised from ξ Hydrae, is a solitary[9] star in the equatorial constellation of Hydra. It was also given the Flamsteed designation 19 Crateris. This magnitude 3.54[2] star is situated 130 light-years from Earth and has a radius about 10 times that of the Sun. It is radiating 58 times as much luminosity as the Sun.[6]

Flamsteed gave Xi Hydrae the designation 19 Crateris. He included a number of stars now within the IAU boundaries of Hydra as part of a Hydra & Crater constellation overlapping parts of both modern constellations.[10]

The star Xi Hydrae is particularly interesting in the field of asteroseismology since it shows solar-like oscillations. Multiple frequency oscillations are found with periods between 2.0 and 5.5 hours.[11]

Xi Hydrae has left the main sequence, having exhausted the supply of hydrogen in its core. Its spectrum is that of a red giant. Modelling its physical properties against theoretical evolutionary tracks shows that it has just reached the foot of the red giant branch for a star with an initial mass around 3 M. This puts its age at about 510 myr.[12]

References

  1. 1.0 1.1 1.2 1.3 1.4 van Leeuwen, F. (2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics 474 (2): 653–664, doi:10.1051/0004-6361:20078357, Bibcode2007A&A...474..653V. 
  2. 2.0 2.1 2.2 Mallik, Sushma V. (December 1999), "Lithium abundance and mass", Astronomy and Astrophysics 352: 495–507, Bibcode1999A&A...352..495M. 
  3. 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, Bibcode2012A&A...546A..61D. 
  4. Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters 38 (5): 331, doi:10.1134/S1063773712050015, Bibcode2012AstL...38..331A. 
  5. 5.0 5.1 5.2 5.3 Heiter, U.; Jofré, P.; Gustafsson, B.; Korn, A. J.; Soubiran, C.; Thévenin, F. (2015), "Gaia FGK benchmark stars: Effective temperatures and surface gravities", Astronomy & Astrophysics 582: A49, doi:10.1051/0004-6361/201526319, Bibcode2015A&A...582A..49H. 
  6. 6.0 6.1 6.2 6.3 Bruntt, H. et al. (July 2010), "Accurate fundamental parameters for 23 bright solar-type stars", Monthly Notices of the Royal Astronomical Society 405 (3): 1907–1923, doi:10.1111/j.1365-2966.2010.16575.x, Bibcode2010MNRAS.405.1907B. 
  7. "URANOMETRIA ARGENTINA". http://www.uranometriaargentina.com/. 
  8. "ksi Hya". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=ksi+Hya. 
  9. 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, doi:10.1111/j.1365-2966.2008.13596.x, Bibcode2008MNRAS.389..869E. 
  10. Wagman, M. (August 1987), "Flamsteed's Missing Stars", Journal for the History of Astronomy 18 (3): 216, doi:10.1177/002182868701800305, Bibcode1987JHA....18..209W. 
  11. Frandsen, S.; Carrier, F.; Aerts, C.; Stello, D.; Maas, T.; Burnet, M.; Bruntt, H.; Teixeira, T. C. et al. (2002). "Detection of Solar-like oscillations in the G7 giant star ξ Hya". Astronomy and Astrophysics 394: L5–L8. doi:10.1051/0004-6361:20021281. Bibcode2002A&A...394L...5F. 
  12. Thévenin, F.; Kervella, P.; Pichon, B.; Morel, P.; Di Folco, E.; Lebreton, Y. (2005). "VLTI/VINCI diameter constraints on the evolutionary status of δ Eri, ξ Hya, η Boo". Astronomy and Astrophysics 436 (1): 253. doi:10.1051/0004-6361:20042075. Bibcode2005A&A...436..253T. 

External links