Star in the constellation Hydra
Eta Hydrae (η Hydrae ) is a star in the equatorial constellation of Hydra . With an apparent visual magnitude of 4.3,[ 2] it is visible to the naked eye. However, it is the faintest of the five stars that form the "head" of the hydra.[ 11] Based upon an annual parallax shift of 5.56 mas ,[ 1] it is located roughly 590 light years from the Sun .
A light curve for Eta Hydrae, plotted from TESS data[ 12]
This is a B-type main sequence star with a stellar classification of B3V.[ 3] It has been classified as a candidate Beta Cephei variable with a period of 2.2 days, although this designation was rejected by Stankov and Handler (2005).[ 4] The spectrum shows a slight underabundance of carbon, compared to the Sun.[ 13] The star is around 32[ 6] million years old and is spinning with a projected rotational velocity of 101[ 9] km/s. It has an estimated seven[ 6] times the mass of the Sun and nearly four[ 7] times the Sun's radius . Eta Hydrae radiates 2,680[ 8] times the solar luminosity from its outer atmosphere at an effective temperature of 18,630[ 9] K.
Name and etymology
This star, along with δ Hya (Lisan al Sudja), ε Hya , ζ Hya , ρ Hya and σ Hya (Minchir), were Ulug Beg's Min al Azʽal , "Belonging to the Uninhabited Spot".[ 14] According to the catalogue of stars in the Technical Memorandum 33-507 - A Reduced Star Catalog Containing 537 Named Stars , Min al Azʽal or Minazal were the title for five stars:δ Hya as Minazal I , η Hya as Minazal II , ε Hya as Minazal III , ρ Hya as Minazal IV and ζ Hya as Minazal V (exclude σ Hya ).[ 15]
In Chinese , 柳宿 (Liǔ Sù ), meaning Willow , refers to an asterism consisting of η Hydrae, δ Hydra , σ Hydrae , ρ Hydrae , ε Hydrae , ζ Hydrae , ω Hydrae and θ Hydrae [ 16] Consequently, η Hydrae itself is known as 柳宿三 (Liǔ Sù sān , English: the Third Star of Willow ).[ 17]
The people of Groote Eylandt called Unwala , "The Crab", for the star cluster including this star, δ Hya (Lisan al Sudja), ε Hya , ζ Hya , ρ Hya and σ Hya (Minchir).[ 18]
References
^ a b c d e f van 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 .
^ a b c d Oja, T. (August 1986), "UBV photometry of stars whose positions are accurately known. III", Astronomy and Astrophysics Supplement Series , 65 (2): 405– 409, Bibcode :1986A&AS...65..405O .
^ a b Levenhagen, R. S.; Leister, N. V. (2006), "Spectroscopic Analysis of Southern B and Be Stars", Monthly Notices of the Royal Astronomical Society , 371 (1): 252– 62, arXiv :astro-ph/0606149 , Bibcode :2006MNRAS.371..252L , doi :10.1111/j.1365-2966.2006.10655.x , S2CID 16492030 .
^ a b Stankov, Anamarija; Handler, Gerald (June 2005), "Catalog of Galactic β Cephei Stars", The Astrophysical Journal Supplement Series , 158 (2): 193– 216, arXiv :astro-ph/0506495 , Bibcode :2005ApJS..158..193S , doi :10.1086/429408 , S2CID 119526948 .
^ 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 .
^ a b c d Tetzlaff, N.; et al. (January 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 .
^ a b Pasinetti Fracassini, L. E.; et al. (February 2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS)", Astronomy and Astrophysics , 367 (3rd ed.): 521– 524, arXiv :astro-ph/0012289 , Bibcode :2001A&A...367..521P , doi :10.1051/0004-6361:20000451 , S2CID 425754 .
^ a b Hohle, M. M.; et al. (April 2010), "Masses and luminosities of O- and B-type stars and red supergiants", Astronomische Nachrichten , 331 (4): 349, arXiv :1003.2335 , Bibcode :2010AN....331..349H , doi :10.1002/asna.200911355 , S2CID 111387483 .
^ a b c d e Huang, W.; Gies, D. R. (August 2008), "Stellar Rotation in Field and Cluster B Stars", The Astrophysical Journal , 683 (2): 1045– 1051, arXiv :0805.2133 , Bibcode :2008ApJ...683.1045H , doi :10.1086/590106 , S2CID 18926523 , 1045−1051.
^ "eta Hya" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2017-01-03 .
^ Moore, Patrick (2013), The Observer's Year: 366 Nights of the Universe , The Patrick Moore Practical Astronomy Series, Springer Science & Business Media , p. 79, ISBN 978-1447136132 .
^ "MAST: Barbara A. Mikulski Archive for Space Telescopes" . Space Telescope Science Institute. Retrieved 8 December 2021 .
^ Schnerr, R. S.; et al. (June 2008), "Magnetic field measurements and wind-line variability of OB-type stars", Astronomy and Astrophysics , 483 (3): 857– 867, arXiv :1008.4260 , Bibcode :2008A&A...483..857S , doi :10.1051/0004-6361:20077740 , S2CID 53454915 .
^ Allen, R. H. (1963), Star Names: Their Lore and Meaning (Reprint ed.), New York, NY: Dover Publications Inc, p. 249 , ISBN 0-486-21079-0 , retrieved 2010-12-12
^ Rhoads, Jack W. (November 15, 1971), Technical Memorandum 33-507-A Reduced Star Catalog Containing 537 Named Stars (PDF) , Jet Propulsion Laboratory, California Institute of Technology
^ (in Chinese) 中國星座神話 , written by 陳久金. Published by 台灣書房出版有限公司, 2005, ISBN 978-986-7332-25-7 .
^ (in Chinese) AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 5 月 28 日 Archived 2011-05-22 at the Wayback Machine
^ Selin, Helaine , ed. (1997), Encyclopaedia of the history of science, technology, and medicine in non-western cultures , Dordrecht: Kluwer Academic Publishers, p. 105, ISBN 9780792340669