Gamma Aquarii

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Gamma Aquarii
Location of γ Aquarii (circled)
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]
Distance
164 ± 9 ly
(50 ± 3 pc)
Absolute magnitude (MV)+0.10[5]
Details
Myr
HR 8518, SAO 146044, ADS 15864, WDS J22217-0123A[9]
Database references
SIMBADdata

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

Chinese name for Gamma Aquarii itself is 墳墓二 (Fén Mù èr, English: the Second Star of Tomb).[20]

Properties

In 1978 through 1984,

speckle interferometry,[21][22] and it is listed as such in the 1991 revision of the Bright Star Catalogue.[23] In 2008, P. P. Eggleton and A. A. Tokovinin listed it as a single star in their catalogue of multiplicity.[24]

It presents as an

References

External links