Nu Aquarii
Star in the constellation Aquarius
Nu Aquarii (ν Aqr, ν Aquarii) is the Bayer designation for a star in the equatorial constellation of Aquarius .
With an apparent visual magnitude of 4.52,[ 2] Nu Aquarii is visible to the naked eye. Its distance from Earth, as determined from parallax measurements, is around 159 light-years (49 parsecs ). At an estimated age of 708 million years,[ 5] it has evolved into a giant star with a spectrum that matches a stellar classification of G8 III.[ 3] It has than double the mass of the Sun [ 5] and has expanded to eight[ 4] times the Sun's radius . Nu Aquarii is radiating 37-fold[ 4] the luminosity of the Sun from its outer atmosphere at an effective temperature of 4,920 K .[ 4] At this heat, the star is glowing with the yellowish hue of a G-type star .[ 7]
Together with μ Aquarii , it is Albulaan , a name derived from the Arabic term al-bulaʽān (ألبولعان ), meaning "the two swallowers". This star, along with ε Aqr (Albali) and μ Aqr (Albulaan), were al Bulaʽ (البلع )—the Swallower.[ 8] [ 9]
In Chinese , 天壘城 (Tiān Lěi Chéng ), meaning Celestial Ramparts , refers to an asterism consisting of ν Aquarii, ξ Aquarii , 46 Capricorni , 47 Capricorni , λ Capricorni , 50 Capricorni , 18 Aquarii , 29 Capricorni , 9 Aquarii , 8 Aquarii , 14 Aquarii , 17 Aquarii and 19 Aquarii .[ 10] Consequently, the Chinese name for ν Aquarii itself is 天壘城十 (Tiān Lěi Chéng shí , English: the Tenth Star of Celestial Ramparts ).[ 11]
References
^ a b c d e 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 .
^ a b c d Johnson, H. L.; et al. (1966), "UBVRIJKL photometry of the bright stars", Communications of the Lunar and Planetary Laboratory , 4 (99): 99, Bibcode :1966CoLPL...4...99J .
^ a b Buscombe, W. (1962), "Spectral classification of Southern fundamental stars", Mount Stromlo Observatory Mimeogram , 4 : 1, Bibcode :1962MtSOM...4....1B .
^ a b c d e f g h i j Massarotti, Alessandro; et al. (January 2008), "Rotational and Radial Velocities for a Sample of 761 HIPPARCOS Giants and the Role of Binarity", The Astronomical Journal , 135 (1): 209–231, Bibcode :2008AJ....135..209M , doi :10.1088/0004-6256/135/1/209 .
^ a b c d e Takeda, Yoichi; Sato, Bun'ei; Murata, Daisuke (August 2008), "Stellar parameters and elemental abundances of late-G giants", Publications of the Astronomical Society of Japan , 60 (4): 781–802, arXiv :0805.2434 , Bibcode :2008PASJ...60..781T , doi :10.1093/pasj/60.4.781 , S2CID 16258166 .
^ "nu. Aqr" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2012-07-02 .
^ "The Colour of Stars" , Australia Telescope, Outreach and Education , Commonwealth Scientific and Industrial Research Organisation , December 21, 2004, archived from the original on December 3, 2013, retrieved 2012-07-02 .
^ Davis Jr., G. A. (October 1944), "The Pronunciations, Derivations, and Meanings of a Selected List of Star Names", Popular Astronomy , 52 (3): 12, Bibcode :1944PA.....52....8D .
^ Allen, R. H. (1963), Star Names: Their Lore and Meaning (Reprint ed.), New York: Dover Publications Inc, p. 53 , ISBN 0-486-21079-0 , retrieved 2010-12-12 .
^ (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) AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 5 月 15 日
External links