  | |
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Aquarius |
| Right ascension | 21h 09m 35.64888s[1] |
| Declination | –11° 22′ 18.0851″[1] |
| Apparent magnitude (V) | 4.52[2] |
| Characteristics | |
| Spectral type | G8 III[3] |
| U−B color index | +0.66[2] |
| B−V color index | +0.94[2] |
| Astrometry | |
| Radial velocity (Rv) | −11.23[4] km/s |
| Proper motion (μ) | RA: +94.12[1] mas/yr Dec.: −14.62[1] mas/yr |
| Parallax (π) | 20.47 ± 0.21 mas[1] |
| Distance | 159 ± 2 ly (48.9 ± 0.5 pc) |
| Absolute magnitude (MV) | +0.93[5] |
| Details | |
| Mass | 2.35[5] M☉ |
| Radius | 8[4] R☉ |
| Luminosity | 37[4] L☉ |
| Surface gravity (log g) | 2.8[4] cgs |
| Temperature | 4,920[4] K |
| Metallicity [Fe/H] | −0.15[4] dex |
| Rotational velocity (v sin i) | 0.0[4] km/s |
| Age | 708[5] Myr |
| Other designations | |
| Database references | |
| SIMBAD | data |
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 /ˌælbjəˈlɑːn/, 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
[edit]- ^ 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
Well, that’s interesting to know that Psilotum nudum are known as whisk ferns. Psilotum nudum is the commoner species of the two. While the P. flaccidum is a rare species and is found in the tropical islands. Both the species are usually epiphytic in habit and grow upon tree ferns. These species may also be terrestrial and grow in humus or in the crevices of the rocks.
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