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C o o r d i n a t e s : 22 h 05 m 4 7 . 0 3 5 9 3 s , − 0 0 ° 1 9 ′ 1 1 . 4 5 6 8 ″
F r o m W i k i p e d i a , t h e f r e e e n c y c l o p e d i a
( R e d i r e c t e d f r o m Α A q u a r i i )
Star in the constellation Aquarius
Alpha Aquarii
Location of α Aquarii (circled)
Observation dataEpoch J2000.0 Equinox J2000.0 (ICRS )
Constellation
Aquarius
Right ascension
22 h 05 m 47.03555s [1]
Declination
−00° 19 ′ 11.4634″[1]
Apparent magnitude (V )
2.942[2]
Characteristics
Spectral type
G2 Ib [3]
U−B color index
+0.699[2]
B−V color index
+0.971[2]
R−I color index
+0.49[2]
Astrometry Radial velocity (R v )7.5[4] km/s Proper motion (μ) RA: +18.59 mas /yr [1] Dec.: −10.45 mas /yr [1] Parallax (π)4.9451 ± 0.4296 mas [1] Distance 690.8+37.8 −56.1 ly ( 211.9+11.6 −17.2 pc )[5] Absolute magnitude (M V )−3.882[6]
Details Mass 6.31[7] M ☉ Radius 83 [7] R ☉ Luminosity 3,917[7] L ☉ Surface gravity (log g )1.4[7] cgs Temperature 5,383± 74 [8] K Metallicity [Fe/H]+0.17[6] dex Rotational velocity (v sin i ) 6.7± 1.5[9] km/sAge 53 [3] Myr
Other designations
El Melik, Rucbah, Saad el Melik, Sadalmelek, Sadalmelik, Sadlamulk, α Aqr, Alpha Aquarii, Alpha Aqr , 34 Aquarii, 34 Aqr , BD −01 4246 , FK5 827, Gaia DR2 2680356911815074432 , HD 209750, HIP 109074, HR 8414, SAO 145862, WDS 22058-0019 , 2MASS J22054703-0019114[10] [11] [12] [13]
Database references SIMBAD data
Alpha Aquarii , officially named Sadalmelik (),[14] is a single star in the constellation of Aquarius . The apparent visual magnitude of 2.94[2] makes this the second-brightest star in Aquarius. Based upon parallax measurements made by the Gaia spacecraft, it is located at a distance of roughly 690 light-years (210 parsecs ) from the Sun .[5] It is drifting further away from the Sun with a radial velocity of 7.5 km/s.[4]
It forms the primary or 'A' component of a double star designated WDS J22058-0019; the secondary or 'B' component is UCAC2 31789179 .[15]
Nomenclature
[ edit ]
α Aquarii (Latinised to Alpha Aquarii ) is the star's Bayer designation . WDS J22058-0019 A is its designation in the Washington Double Star Catalog .
It bore the traditional name Sadalmelik , which derived from an Arabic expression سعد الملك (sa‘d al-malik ), meaning "Luck of the king". The name Rucbah had also been applied to this star; though it shared that name with Delta Cassiopeiae .[13] It is only one of two stars with ancient proper names to lie within a degree of the celestial equator . The origin of the Arabic name is lost to history.[16] In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN)[17] to catalogue and standardize proper names for stars. The WGSN approved the name Sadalmelik for Alpha Aquarii (WDS J22058-0019 A) on 21 August 2016, and it is now so included in the List of IAU-approved Star Names (Delta Cassiopeiae was given the name Ruchbah ).[14]
In Chinese , 危宿 (Wēi Xiù ), meaning Rooftop (asterism) , refers to an asterism consisting of Alpha Aquarii, Theta Pegasi and Epsilon Pegasi .[18] Consequently, the Chinese name for Alpha Aquarii itself is 危宿一 (Wēi Xiù yī , English: the First Star of Rooftop ).[19]
Properties
[ edit ]
With an age of 53 million years,[3] Alpha Aquarii has evolved into a supergiant with a stellar classification of G2 Ib.[3] It lies within the Cepheid instability strip of the Hertzsprung–Russell diagram , near the red (cooler) edge, but is not classified as a variable star . However, variable cores have been detected in the hydrogen lines , which are originating in a circumstellar envelope.[20] The star has a massive stellar wind that reaches supersonic velocity in the chromosphere .[21]
There is some uncertainty about Alpha Aquarii's distance. The original Hipparcos catalog gave a parallax of 4.3± 0.83 mas , which translates to a distance of 233± 45 parsecs , or 760 light-years .[22] The 2007 Hipparcos reduction gave a parallax of 6.23± 0.19 milliarcseconds , translating into a distance of 161± 5 pc , or 520 light-years.[23] Measurements by the Gaia spacecraft on its second data release (DR2 ) give a parallax of 12.9± 0.8 mas , giving a much lower distance of 77.5± 4.8 pc (250 ly).[24] The third Gaia data release (Gaia DR3 ) give a parallax of 4.94± 0.43 mas , translating to a distance of 202± 17 pc , or 660 light-years .[1]
Alpha Aquarii has 6.3 times as much mass as the Sun and has expanded to around 80 times the Sun's radius . It is radiating 3,900 times as much luminosity as the Sun from its outer atmosphere [7] at an effective temperature of 5,383 K .[8] At this heat, the star glows with the yellow hue of a G-type star .[25] Examination of this star with the Chandra X-ray Observatory shows it to be significantly X-ray deficient compared to G-type main-sequence stars . This deficit is a common feature of early G-type giant stars.[9]
The visual companion (UCAC2 31789179) has an apparent visual magnitude of approximately 12.2. It is at an angular separation of 110.4 arcseconds from Alpha Aquarii along a position angle of 40°.[12]
References
[ edit ]
^ a b c d e Cousins, A. W. J. (1984), "Standardization of Broadband Photometry of Equatorial Standards", South African Astronomical Observatory Circulars , 8 : 59, Bibcode :1984SAAOC...8...59C
^ a b c d Lyubimkov, Leonid S.; et al. (February 2010), "Accurate fundamental parameters for A-, F- and G-type Supergiants in the solar neighbourhood", Monthly Notices of the Royal Astronomical Society , 402 (2 ): 1369–1379, arXiv :0911.1335 , Bibcode :2010MNRAS.402.1369L , doi :10.1111/j.1365-2966.2009.15979.x , S2CID 119096173
^ a b Wielen, R.; et al. (1999), "Sixth Catalogue of Fundamental Stars (FK6). Part I. Basic fundamental stars with direct solutions", Veröff. Astron. Rechen-Inst. Heidelb , 35 (35 ), Astronomisches Rechen-Institut Heidelberg: 1, Bibcode :1999VeARI..35....1W
^ a b Bailer-Jones, C. A. L.; Rybizki, J.; Fouesneau, M.; Demleitner, M.; Andrae, R. (2021-03-01). "Estimating distances from parallaxes. V: Geometric and photogeometric distances to 1.47 billion stars in Gaia Early Data Release 3" . The Astronomical Journal . 161 (3 ): 147. arXiv :2012.05220 . Bibcode :2021AJ....161..147B . doi :10.3847/1538-3881/abd806 . ISSN 0004-6256 . Data about this star can be seen here .
^ a b Soubiran, C.; et al. (2008). "Vertical distribution of Galactic disk stars. IV. AMR and AVR from clump giants". Astronomy and Astrophysics . 480 (1 ): 91–101. arXiv :0712.1370 . Bibcode :2008A&A...480...91S . doi :10.1051/0004-6361:20078788 . S2CID 16602121 .
^ a b c d e Ayres, Thomas (2023-05-01). "In the Trenches of the Solar-Stellar Connection. VII. Wilson-Bappu 2022" . The Astrophysical Journal Supplement Series . 266 (1 ): 6. Bibcode :2023ApJS..266....6A . doi :10.3847/1538-4365/acb535 . ISSN 0067-0049 . Alpha Aquarii's database entry at VizieR .
^ a b Baines, Ellyn K.; et al. (2018). "Fundamental Parameters of 87 Stars from the Navy Precision Optical Interferometer" . The Astronomical Journal . 155 (1 ). 30. arXiv :1712.08109 . Bibcode :2018AJ....155...30B . doi :10.3847/1538-3881/aa9d8b .
^ a b Ayres, Thomas R.; Brown, Alexander; Harper, Graham M. (July 2005), "Chandra Observations of Coronal Emission from the Early G Supergiants α and β Aquarii", The Astrophysical Journal , 627 (1 ): L53–L56, Bibcode :2005ApJ...627L..53A , doi :10.1086/431977 , S2CID 122519436
^ HR 8414 , database entry, The Bright Star Catalogue, 5th Revised Ed. (Preliminary Version), D. Hoffleit and W. H. Warren, Jr., CDS ID V/50 . Accessed on line October 3, 2008.
^ "Alpha Aquarii" . SIMBAD . Centre de données astronomiques de Strasbourg .
^ a b Entry 22058-0019, The Washington Double Star Catalog Archived 2009-01-31 at the Wayback Machine , United States Naval Observatory . Accessed on line November 18, 2008.
^ a b pp. 51, 148, Star-names and Their Meanings , Richard Hinckley Allen, New York: G. E. Stechert, 1899.
^ a b "Naming Stars" . IAU.org. Retrieved 25 February 2018 .
^ "UCAC2 31789179 -- Star" , SIMBAD , Centre de Données astronomiques de Strasbourg, retrieved 2018-02-25
^ Sadalmelik , Stars , Jim Kaler. Accessed on line October 3, 2008.
^ IAU Working Group on Star Names (WGSN) , International Astronomical Union , retrieved 22 May 2016 .
^ (in Chinese) 中國星座神話 , written by 陳久金. Published by 台灣書房出版有限公司, 2005, ISBN 978-986-7332-25-7 .
^ (in Chinese) 香港太空館 - 研究資源 - 亮星中英對照表 Archived 2010-08-18 at the Wayback Machine , Hong Kong Space Museum. Accessed on line November 23, 2010.
^ Usenko, I. A.; et al. (November 2017), "Spectroscopic studies of the unique yellow supergiant α Aqr in the Cepheid instability strip", Astronomy Letters , 43 (11 ): 751–767, Bibcode :2017AstL...43..751U , doi :10.1134/S1063773717110068 , S2CID 41734976 .
^ Dupree, A. K.; et al. (December 1993), "HST/GHRS Spectroscopy of the Hybrid Star Alpha Aquarii", Bulletin of the American Astronomical Society , 25 , American Astronomical Society, 183rd AAS Meeting: 1321, Bibcode :1993AAS...183.1807D , 18.07.
^ ESA (1997-01-01). "The HIPPARCOS and TYCHO catalogues. Astrometric and photometric star catalogues derived from the ESA HIPPARCOS Space Astrometry Mission" . ESA Special Publication . 1200 . ISSN 1609-042X .
^ van Leeuwen, F. (November 2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics , 474 (2 ): 653–664, arXiv :0708.1752 , Bibcode :2007A&A...474..653V , doi :10.1051/0004-6361:20078357 , S2CID 18759600
^ 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 .
^ "The Colour of Stars" , Australia Telescope, Outreach and Education , Commonwealth Scientific and Industrial Research Organisation , December 21, 2004, archived from the original on February 22, 2012, retrieved 2012-01-16
External links
[ edit ]
R e t r i e v e d f r o m " https://en.wikipedia.org/w/index.php?title=Alpha_Aquarii&oldid=1235929437 "
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