Star in the constellation Aquila
20 Aquilae , abbreviated 20 Aql , is an irregular variable [ 11] star in the equatorial constellation of Aquila . 20 Aquilae is its Flamsteed designation . It ranges in magnitude from a peak of 5.33 down to 5.36, which is bright enough for the star to be visible to the naked eye.[ 12] The estimated distance to this star is around 920 light years , based upon an annual parallax shift of 3.5 mas .[ 2] The star is moving closer to the Earth with a heliocentric radial velocity of −23 km/s.[ 7]
There has been some disagreement over the stellar classification of this star. Buscombe (1962) listed a class of B3 IV,[ 5] which suggests a B-type subgiant star that has exhausted the hydrogen at its core and is expanding off the main sequence . Lesh (1968)[ 13] and Braganca et al. (2012)[ 4] matched a B-type main sequence star with a class of B3 V. However, Houk and Swift (1999) found a class of B2/3 II,[ 6] indicating this is an evolved bright giant .
The star is about 28[ 9] million years old with a high rate of spin, showing a projected rotational velocity of 133 km/s.[ 4] It has 8.6[ 9] times the mass of the Sun and is radiating 7,284 times the Sun's luminosity from its photosphere at an effective temperature of 18,700 K.[ 3]
References
^ "Hipparcos Tools Interactive Data Access" . Hipparcos . ESA. Retrieved 8 December 2021 .
^ a b c d e f 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 .
^ a b c d e Hohle, M. M.; et al. (April 2010), "Masses and luminosities of O- and B-type stars and red supergiants", Astronomische Nachrichten , 331 (4): 349, arXiv :1003.2335 , Bibcode :2010AN....331..349H , doi :10.1002/asna.200911355 , S2CID 111387483 .
^ a b c d Bragança, G. A.; et al. (November 2012), "Projected Rotational Velocities and Stellar Characterization of 350 B Stars in the Nearby Galactic Disk", The Astronomical Journal , 144 (5): 10, arXiv :1208.1674 , Bibcode :2012AJ....144..130B , doi :10.1088/0004-6256/144/5/130 , S2CID 118868235 , 130.
^ a b Buscombe, W. (1962), "Spectral classification of Southern fundamental stars", Mount Stromlo Observatory Mimeogram , 4 : 1, Bibcode :1962MtSOM...4....1B .
^ 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 Gontcharov, G. A. (2006), "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system", Astronomy Letters , 32 (11): 759– 771, arXiv :1606.08053 , Bibcode :2006AstL...32..759G , doi :10.1134/S1063773706110065 , S2CID 119231169 .
^ 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 c d Tetzlaff, N.; et al. (January 2011), "A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun", Monthly Notices of the Royal Astronomical Society , 410 (1): 190– 200, arXiv :1007.4883 , Bibcode :2011MNRAS.410..190T , doi :10.1111/j.1365-2966.2010.17434.x , S2CID 118629873 .
^ "20 Aql" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved October 29, 2018 .
^ Lefèvre, L.; Marchenko, S. V.; Moffat, A. F. J.; Acker, A. (2009), "A systematic study of variability among OB-stars based on HIPPARCOS photometry", Astronomy and Astrophysics , 507 (2): 1141– 1201, Bibcode :2009A&A...507.1141L , doi :10.1051/0004-6361/200912304 , ISSN 0004-6361 .
^ Samus, N. N.; et al. (2017), "General Catalogue of Variable Stars", Astronomy Reports , GCVS 5.1, 61 (1): 80– 88, Bibcode :2017ARep...61...80S , doi :10.1134/S1063772917010085 , S2CID 125853869 .
^ Lesh, Janet Rountree (December 1968), "The Kinematics of the Gould Belt: an Expanding Group?", Astrophysical Journal Supplement , 17 : 371, Bibcode :1968ApJS...17..371L , doi :10.1086/190179 .