Star in the constellation Aquarius
26 Aquarii is a single[ 6] star located approximately 960[ 1] light years away from the Sun in the zodiac constellation of Aquarius . 26 Aquarii is the Flamsteed designation .[ 5] It is visible to the naked eye as a dim, orange-hued star with an apparent visual magnitude of 5.66.[ 2] This object is moving away from the Earth with a heliocentric radial velocity of +8 km/s.[ 2]
Houk and Swift (1999) listed a stellar classification of K2(III)[ 3] for 26 Aquarii, corresponding to an evolved K-type giant of uncertain luminosity class . Bartkevicius and Lazauskaite (1997) found spectral traits of MD-Ba?-K3 II–III, K2 Ia , suggesting some type of giant K-type star with a suspected metal deficiency (MD) of barium.[ 7] It has 54.5 times the Sun's radius and is radiating 842 times the luminosity of the Sun from its photosphere at an effective temperature of 4,210 K.[ 1]
References
^ a b c d e f g h i j Brown, A. G. A. ; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties" . Astronomy & Astrophysics . 616 . A1. arXiv :1804.09365 . Bibcode :2018A&A...616A...1G . doi :10.1051/0004-6361/201833051 . Gaia DR2 record for this source at VizieR .
^ a b c d e f Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters , 38 (5): 331, arXiv :1108.4971 , Bibcode :2012AstL...38..331A , doi :10.1134/S1063773712050015 , S2CID 119257644 .
^ a b Houk, N.; Swift, C. (1999), "Michigan catalogue of two-dimensional spectral types for the HD Stars", Michigan Spectral Survey , 5 , Bibcode :1999MSS...C05....0H .
^ a b Rebull, Luisa M.; et al. (October 2015), "On Infrared Excesses Associated with Li-rich K Giants", The Astronomical Journal , 150 (4): 45, arXiv :1507.00708 , Bibcode :2015AJ....150..123R , doi :10.1088/0004-6256/150/4/123 , S2CID 46595131 , 123.
^ a b "26 Aqr" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2019-05-16 .
^ Eggleton, P. P.; Tokovinin, A. A. (2008), "A catalogue of multiplicity among bright stellar systems", Monthly Notices of the Royal Astronomical Society , 389 (2): 869, arXiv :0806.2878 , Bibcode :2008MNRAS.389..869E , doi :10.1111/j.1365-2966.2008.13596.x , S2CID 14878976 .
^ Bartkevicius, A.; Lazauskaite, R. (December 1997), "Classification of Population II Stars in the Vilnius Photometric System. II. Results", Baltic Astronomy , 6 (4): 499– 572, Bibcode :1997BaltA...6..499B , doi :10.1515/astro-1997-0402 .