7 Aquarii
Star in the constellation Aquarius
7 Aquarii , abbreviated 7 Aqr , is a binary star [ 3] system in the zodiac constellation of Aquarius . 7 Aquarii is the Flamsteed designation . It is visible to the naked eye with an apparent visual magnitude of 5.5;[ 2] the brighter component is baseline magnitude 5.62 while the faint secondary is magnitude 11.4.[ 3] As of 2002, the pair had an angular separation of 2.10″ along a position angle of 165°.[ 10] The distance to this system, based upon an annual parallax shift of 4.9 mas ,[ 1] is around 660 light years . It is moving closer to the Earth with a heliocentric radial velocity of −32 km/s.[ 7]
The primary component is an aging giant star with a stellar classification of K4 III.[ 4] It is a suspected variable star of unknown type with a maximum magnitude of 5.48.[ 6] The interferometry -measured angular diameter of this star, after correcting for limb darkening , is 2.14± 0.02 mas ,[ 11] which, at its estimated distance, equates to a physical radius of about 46 times the radius of the Sun .[ 8] The star is radiating 404[ 5] times the Sun's luminosity from its enlarged photosphere at an effective temperature of 3,990 K.[ 2]
References
^ 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 f McWilliam, Andrew (December 1990), "High-resolution spectroscopic survey of 671 GK giants. I. Stellar atmosphere parameters and abundances", Astrophysical Journal Supplement Series , 74 : 1075–1128, Bibcode :1990ApJS...74.1075M , doi :10.1086/191527 .
^ a b c Eggleton, P. P.; Tokovinin, A. A. (September 2008), "A catalogue of multiplicity among bright stellar systems", Monthly Notices of the Royal Astronomical Society , 389 (2): 869–879, arXiv :0806.2878 , Bibcode :2008MNRAS.389..869E , doi :10.1111/j.1365-2966.2008.13596.x , S2CID 14878976 .
^ a b Houk, Nancy; Smith-Moore, M. (1978), Michigan catalogue of two-dimensional spectral types for the HD stars , vol. 4, Ann Arbor: Dept. of Astronomy, University of Michigan, Bibcode :1988mcts.book.....H .
^ a b c d 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 Samus, N. N.; Kazarovets, E. V.; Durlevich, O. V.; Kireeva, N. N.; Pastukhova, E. N. (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 .
^ 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 .
^ a b Lang, Kenneth R. (2006), Astrophysical formulae , Astronomy and astrophysics library, vol. 1 (3rd ed.), Birkhäuser , ISBN 3-540-29692-1 . The radius (R* ) is given by:
2
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10
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3
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202
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2.14
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0.0046491
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R
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93
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{\displaystyle {\begin{aligned}2\cdot R_{*}&={\frac {(10^{-3}\cdot 202\cdot 2.14)\ {\text{AU}}}{0.0046491\ {\text{AU}}/R_{\bigodot }}}\\&\approx 93\cdot R_{\bigodot }\end{aligned}}}
^ "7 Aqr" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved October 22, 2018 .
^ Mason, B. D.; et al. (2014), "The Washington Visual Double Star Catalog", The Astronomical Journal , 122 (6): 3466, Bibcode :2001AJ....122.3466M , doi :10.1086/323920 .
^ Richichi, A.; et al. (February 2005), "CHARM2: An updated Catalog of High Angular Resolution Measurements", Astronomy and Astrophysics , 431 (2): 773–777, Bibcode :2005A&A...431..773R , doi :10.1051/0004-6361:20042039 .
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