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Star in the constellation Aquila
64 Aquilae , abbreviated 64 Aql , is a star in the equatorial constellation of Aquila . 64 Aquilae is its Flamsteed designation . It is a faint star that requires good viewing conditions to see, having an apparent visual magnitude of 5.97. The distance to 64 Aql, as determined from its annual parallax shift of 21.42 mas , is 152.2 light years . At that distance, the visual magnitude of the star is diminished by an extinction of 0.029 due to interstellar dust . It is moving closer to the Earth with a heliocentric radial velocity of −3.6 km/s.
This is an evolved giant star currently on the red giant branch with a stellar classification of K1 III/IV. The luminosity class of 'III/IV' indicates the spectrum shows a blend of features matching a subgiant and giant star. It is around 6.2 billion years old with 1.17 times the mass of the Sun and has expanded to 4.5 times the Sun's radius . The star is radiating 11 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,786 K.
References
^ 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 .
^ 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 .
^ Houk, N.; Swift, C. (1999), "Michigan catalogue of two-dimensional spectral types for the HD Stars", Michigan Spectral Survey , 5 , Bibcode :1999MSS...C05....0H .
^ Maldonado, J.; et al. (June 2013), "The metallicity signature of evolved stars with planets", Astronomy & Astrophysics , 554 : 18, arXiv :1303.3418 , Bibcode :2013A&A...554A..84M , doi :10.1051/0004-6361/201321082 , S2CID 119289111 , A84.
^ Jones, M. I.; et al. (December 2011), "Study of the impact of the post-MS evolution of the host star on the orbits of close-in planets. I. Sample definition and physical properties", Astronomy & Astrophysics , 536 : 7, arXiv :1110.6459 , Bibcode :2011A&A...536A..71J , doi :10.1051/0004-6361/201117887 , S2CID 55769003 , A71.
"64 Aql" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved November 1, 2018.
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