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Theta Aquarii

From Wikipedia, the free encyclopedia
Star in the constellation Aquarius
"Ancha" redirects here; not to be confused withAnkaa.
θ Aquarii
Location of θ Aquarii (circled)
Observation data
Epoch J2000      Equinox J2000
ConstellationAquarius
Right ascension22h 16m 50.03635s[1]
Declination–07° 46′ 59.8480″[1]
Apparent magnitude (V)4.175[2]
Characteristics
Spectral typeG8 III–IV[3]
U−Bcolor index+0.818[2]
B−Vcolor index+0.983[2]
Astrometry
Radial velocity (Rv)–13.77 ± 0.17[4] km/s
Proper motion (μ)RA: +118.80[1]mas/yr
Dec.: –22.18[1]mas/yr
Parallax (π)17.40±0.23 mas[1]
Distance187 ± 2 ly
(57.5 ± 0.8 pc)
Absolute magnitude (MV)+0.23[3]
Details
Mass2.39[5] to 2.78[3] M
Radius12[4] R
Luminosity72[4] to 83[3] L
Surface gravity (log g)2.8[4] cgs
Temperature4,864[4] K
Metallicity [Fe/H]+0.01[4] to +0.09[3] dex
Rotational velocity (v sin i)1.6[4] km/s
Age437[3] Myr
Other designations
Ancha, 43 Aquarii,BD–08 5845,FK5 840,HD 211391,HIP 110003,HR 8499,SAO 145991.[6]
Database references
SIMBADdata

Theta Aquarii (θ Aquarii, abbreviatedTheta Aqr,θ Aqr), officially namedAncha/ˈæŋkə/[7] (distinguishAnkaa, with the same pronunciation), is astar in theequatorialconstellation ofAquarius. Visible to the naked eye atapparent magnitude 4.175,[2] it is located at a distance of around 187light-years (57parsecs) from theSun.[1] Since it is near theecliptic it can beocculted by theMoon, or very rarely byplanets.

Nomenclature

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θ Aquarii (Latinised toTheta Aquarii) is the star'sBayer designation.

It bore the traditional nameAncha;Medieval Latin for "thehaunch". In 2016, theInternational Astronomical Union organized aWorking Group on Star Names (WGSN)[8] to catalogue and standardize proper names for stars. The WGSN approved the nameAncha for this star on 12 September 2016, and it is now so included in the List of IAU-approved Star Names.[7]

InChinese, (), meaningWeeping, refers to anasterism consisting of Theta Aquarii andRho Aquarii.[9] Consequently, theChinese name for Theta Aquarii itself is泣二 (Qì èr, English:the Second Star of Weeping).[10] Possibly, the nameLei, meaning "tears (weeping)" in Chinese, derives from the Chinese name for this star.[11]

Properties

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Ancha belongs to thespectral class G8 with aluminosity class of III–IV suggesting that, at an age of 437[3] million years, this star is part way between thesubgiant andgiant stages of itsevolution. Estimates of the star's mass range from 2.39[5] to 2.78[3] timesthe Sun's mass, with a radius of about 12[4] times thatof the Sun. It is radiating from 72[4] to 83[3] times as much luminosityas the Sun from its enlargedouter envelope at aneffective temperature of 4,864 K.[4] At this heat, the star glows with the yellow hue of aG-type star.[12]

References

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  1. ^abcdefvan Leeuwen, F. (November 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. ^abcdGutierrez-Moreno, Adelina; et al. (1966). "A System of photometric standards".Publications of the Department of Astronomy University of Chile.1. Publicaciones Universidad de Chile, Department de Astronomy:1–17.Bibcode:1966PDAUC...1....1G.
  3. ^abcdefghiTakeda, Yoichi; et al. (August 2008), "Stellar Parameters and Elemental Abundances of Late-G Giants",Publications of the Astronomical Society of Japan,60 (4):781–802,arXiv:0805.2434,Bibcode:2008PASJ...60..781T,doi:10.1093/pasj/60.4.781,S2CID 16258166.
  4. ^abcdefghijMassarotti, Alessandro; et al. (January 2008), "Rotational and Radial Velocities for a Sample of 761 HIPPARCOS Giants and the Role of Binarity",The Astronomical Journal,135 (1):209–231,Bibcode:2008AJ....135..209M,doi:10.1088/0004-6256/135/1/209.
  5. ^abPizzolato, N.; Maggio, A.; Sciortino, S. (September 2000), "Evolution of X-ray activity of 1-3 Msun late-type stars in early post-main-sequence phases",Astronomy and Astrophysics,361:614–628,Bibcode:2000A&A...361..614P.
  6. ^"* tet Aqr".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2012-06-30.
  7. ^ab"Naming Stars". IAU.org. Retrieved16 December 2017.
  8. ^IAU Working Group on Star Names (WGSN),International Astronomical Union, retrieved22 May 2016.
  9. ^(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.
  10. ^(in Chinese)香港太空館 - 研究資源 - 亮星中英對照表Archived 2010-08-11 at theWayback Machine, Hong Kong Space Museum. Accessed on line November 23, 2010.
  11. ^Richard Hinckley Allen."Star Names — Their Lore and Meaning".www.constellationsofwords.com.
  12. ^"The Colour of Stars",Australia Telescope, Outreach and Education, Commonwealth Scientific and Industrial Research Organisation, December 21, 2004, archived fromthe original on 2013-12-03, retrieved2012-01-16.

External links

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