Gamma Aquarii
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Aquarius |
Right ascension | 22h 21m 39.37542s[1] |
Declination | –01° 23′ 14.4031″[1] |
Apparent magnitude (V) | 3.849[2] |
Characteristics | |
Spectral type | A0 V[3] |
U−B color index | –0.092[2] |
B−V color index | –0.060[2] |
Absolute magnitude (MV) | +0.10[5] |
Details | |
Myr | |
Database references | |
SIMBAD | data |
Gamma Aquarii, or γ Aquarii, is a suspected binary star system in the constellation of Aquarius. It has an apparent visual magnitude of 3.849,[2] making it one of the brighter members of the constellation. Based upon parallax measurements taken during the Hipparcos mission, this star is located at a distance of approximately 164 light-years (50 parsecs) from the Sun.[1] It is drifting closer to the Sun with a radial velocity of −16 km/s.[4] In 1998, Olin J. Eggen included this star as a candidate member of the Hyades Supercluster.[5]
Gamma Aquarii is the primary or 'A' component of a double star designated WDS J22217-0123.[10] The secondary or 'B' component is UCAC2 31430071.[11] Gamma Aquarii A's two purported components are therefore designated WDS J22217-0123 Aa and Ab. Gamma Aquarii is traditionally also called Sadachbia /səˈdækbiə/,[12] a name now formally restricted to γ Aqr Aa.[13]
Nomenclature
γ Aquarii, Latinised to Gamma Aquarii, is the system's Bayer designation. WDS J22217-0123 A is its designation in the Washington Double Star Catalog.
It bore the traditional name Sadachbia, from an Arabic expression سعد الأخبية (sa‘d al-’axbiyah), meaning "luck of the homes (tents)". In Hindi it is also called Satabhishaj (a hundred physicians); it is called Sadhayam in Tamil. In the catalogue of stars in the Calendarium of Al Achsasi Al Mouakket, this star was designated Aoul al Achbiya (أول ألأجبية - awwil al ahbiyah), which was translated into Latin as Prima Tabernaculorum, meaning the first of luck of the homes (tents).[14] In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN)[15] to catalogue and standardize proper names for stars. The WGSN approved the name Sadachbia for the component WDS J22217-0123 Aa on 21 August 2016, and it is now so included in the List of IAU-approved Star Names.[13]
This star, along with Pi Aquarii (Seat), Zeta Aquarii (Sadaltager / Achr al Achbiya) and Eta Aquarii (Hydria), were al Aḣbiyah الأخبية "the Tent".[16][17][18]
In
Properties
In 1978 through 1984,
It presents as an
References
- ^ S2CID 18759600.
- ^ Bibcode:1984SAAOC...8...59C.
- ^ doi:10.1086/110819.
- ^ S2CID 119231169.
- ^ doi:10.1086/300413.
- ^ S2CID 33401607. Vizier catalog entry
- ^ doi:10.1086/149890.
- ^ S2CID 18475298.
- ^ "gam Aqr". SIMBAD. Centre de données astronomiques de Strasbourg.
{{cite web}}
: CS1 maint: postscript (link) - ^ "Washington Double Star Catalog". United States Naval Observatory. Archived from the original on 14 February 2011. Retrieved 26 February 2018.
- ^ "UCAC2 31430071". SIMBAD. Centre de données astronomiques de Strasbourg.
{{cite web}}
: CS1 maint: postscript (link) - ISBN 978-1-931559-44-7.
- ^ a b "Naming Stars". IAU.org. Retrieved 26 February 2018.
- .
- ^ IAU Working Group on Star Names (WGSN), International Astronomical Union, retrieved 22 May 2016.
- Bibcode:1944PA.....52....8D
- ISBN 0-486-21079-0, retrieved 2010-12-12.
- Hebrew)
- ISBN 978-986-7332-25-7.
- ^ (in Chinese) 香港太空館 - 研究資源 - 亮星中英對照表 Archived August 18, 2010, at the Wayback Machine, Hong Kong Space Museum. Accessed on line November 23, 2010.
- doi:10.1086/130327.
- S2CID 122218502.
- Bibcode:1964cbs..book.....H.
- S2CID 14878976.
- .
- , 39.
- Commonwealth Scientific and Industrial Research Organisation, December 21, 2004, archived from the originalon 2012-03-18, retrieved 2012-01-16.