Altair (//) designated α Aquilae (Latinised to Alpha Aquilae, abbreviated Alpha Aql, α Aql), is the brightest star in the constellation of Aquila and the twelfth brightest star in the night sky. It is currently in the G-cloud—a nearby interstellar cloud, an accumulation of gas and dust. Altair is an A-type main sequence star with an apparent visual magnitude of 0.77 and is one of the vertices of the Summer Triangle asterism (the other two vertices are marked by Deneb and Vega). It is 16.7 light-years (5.13 parsecs) from the Sun and is one of the most visible stars to the naked eye.
Epoch J2000.0 Equinox J2000.0 (ICRS)
|Right ascension||19h 50m 46.99855s|
|Declination||+08° 52′ 05.9563″|
|Apparent magnitude (V)||0.76|
|Evolutionary stage||Main sequence|
|U−B color index||+0.09|
|B−V color index||+0.22|
|V−R color index||+0.14|
|R−I color index||+0.13|
|Variable type||Delta Scuti|
|Radial velocity (Rv)||−26.1 ± 0.9 km/s|
|Proper motion (μ)|| RA: +536.23 mas/yr |
Dec.: +385.29 mas/yr
|Parallax (π)||194.95 ± 0.57 mas|
|Distance||16.73 ± 0.05 ly |
(5.13 ± 0.01 pc)
|Absolute magnitude (MV)||2.22|
|Mass||1.79 ± 0.018 M☉|
|Radius||1.63 to 2.03[nb 1] R☉|
|Surface gravity (log g)||4.29 cgs|
|Temperature||6,900 to 8,500[nb 1] K|
|Metallicity [Fe/H]||−0.2 dex|
|Rotational velocity (v sin i)||240 km/s|
Altair rotates rapidly, with a velocity at the equator of approximately 286 km/s.[nb 2] This is a significant fraction of the star's estimated breakup speed of 400 km/s. A study with the Palomar Testbed Interferometer revealed that Altair is not spherical, but is flattened at the poles due to its high rate of rotation. Other interferometric studies with multiple telescopes, operating in the infrared, have imaged and confirmed this phenomenon.
α Aquilae (Latinised to Alpha Aquilae) is the star's Bayer designation. The traditional name Altair has been used since medieval times. It is an abbreviation of the Arabic phrase النسر الطائر (the right, first word having forms from Al Nesr, ranging to An-nisr) Al-ta'ir, "the flying (eagle)".
In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN) to catalog and standardize proper names for stars. The WGSN's first bulletin of July 2016 included a table of the first two batches of names approved by the WGSN, which included Altair for this star. It is now so entered in the IAU Catalog of Star Names.
Altair is a type-A main sequence star with about 1.8 times the mass of the Sun and 11 times of its luminosity. Altair rotates rapidly, with a rotational period of about 9 hours; for comparison, the equator of the Sun makes a complete rotation in a little more than 25 days. Its rapid rotation forces the star to be oblate; its equatorial diameter is over 20 percent greater than its polar diameter.
Satellite measurements made in 1999 with the Wide Field Infrared Explorer showed that the brightness of Altair fluctuates slightly, varying by just a few thousandths of a magnitude with several different periods less than 2 hours. As a result, it was identified in 2005 as a Delta Scuti variable star. Its light curve can be approximated by adding together a number of sine waves, with periods that range between 0.8 and 1.5 hours. It is a weak source of coronal X-ray emission, with the most active sources of emission being located near the star's equator. This activity may be due to convection cells forming at the cooler equator.
The angular diameter of Altair was measured interferometrically by R. Hanbury Brown and his co-workers at Narrabri Observatory in the 1960s. They found a diameter of 3 milliarcseconds. Although Hanbury Brown et al. realized that Altair would be rotationally flattened, they had insufficient data to experimentally observe its oblateness. Altair was later observed to be flattened by infrared interferometric measurements made by the Palomar Testbed Interferometer in 1999 and 2000. This work was published by G. T. van Belle, David R. Ciardi and their co-authors in 2001.
Theory predicts that, owing to Altair's rapid rotation, its surface gravity and effective temperature should be lower at the equator, making the equator less luminous than the poles. This phenomenon, known as gravity darkening or the von Zeipel effect, was confirmed for Altair by measurements made by the Navy Prototype Optical Interferometer in 2001, and analyzed by Ohishi et al. (2004) and Peterson et al. (2006). Also, A. Domiciano de Souza et al. (2005) verified gravity darkening using the measurements made by the Palomar and Navy interferometers, together with new measurements made by the VINCI instrument at the VLTI.
Altair is one of the few stars for which a direct image has been obtained. In 2006 and 2007, J. D. Monnier and his coworkers produced an image of Altair's surface from 2006 infrared observations made with the MIRC instrument on the CHARA array interferometer; this was the first time the surface of any main-sequence star, apart from the Sun, had been imaged. The false-color image was published in 2007. The equatorial radius of the star was estimated to be 2.03 solar radii, and the polar radius 1.63 solar radii—a 25% increase of the stellar radius from pole to equator. The polar axis is inclined by about 60° to the line of sight from the Earth.
Etymology, mythology, and cultureEdit
The term Al Nesr Al Tair appeared in Al Achsasi al Mouakket's catalogue, which was translated into Latin as Vultur Volans. This name was applied by the Arabs to the asterism of Altair, β Aquilae, and γ Aquilae and probably goes back to the ancient Babylonians and Sumerians, who called Altair "the eagle star". The spelling Atair has also been used. Medieval astrolabes of England and Western Europe depicted Altair and Vega as birds.
The Koori people of Victoria also knew Altair as Bunjil, the wedge-tailed eagle, and β and γ Aquilae are his two wives the black swans. The people of the Murray River knew the star as Totyerguil. The Murray River was formed when Totyerguil the hunter speared Otjout, a giant Murray cod, who, when wounded, churned a channel across southern Australia before entering the sky as the constellation Delphinus.
In Chinese belief, the asterism consisting of Altair, β Aquilae, and γ Aquilae is known as Hé Gǔ (河鼓; lit. "river drum"). The Chinese name for Altair is thus Hé Gǔ èr (河鼓二; lit. "river drum two", meaning the "second star of the drum at the river"). However, Altair is better known by its other names: Qiān Niú Xīng (牵牛星 / 牽牛星) or Niú Láng Xīng (牛郎星), translated as the cowherd star. These names are an allusion to a love story, The Cowherd and the Weaver Girl, in which Niulang (represented by Altair) and his two children (represented by β Aquilae and γ Aquilae) are separated from respectively their wife and mother Zhinu (represented by Vega) by the Milky Way. They are only permitted to meet once a year, when magpies form a bridge to allow them to cross the Milky Way.
The bright primary star has the multiple star designation WDS 19508+0852A and has several faint visual companion stars, WDS 19508+0852B, C, D, E, F, and G. All are much more distant than Altair and not physically associated.
|B||A||19h 50m 40.5s||+08° 52′ 13″||2015||195.8″||286°||9.8||SIMBAD|
|C||A||19h 51m 00.8s||+08° 50′ 58″||2015||186.4″||110°||10.3||SIMBAD|
|F||A||19h 51m 02.0s||+08° 55′ 33″||2015||292.4″||48°||10.3||SIMBAD|
- Owing to its rapid rotation, Altair's radius is larger at its equator than at its poles; it is also cooler at the equator than at the poles.
- From values of v sin i and i in the second column of Table 1, Monnier et al. 2007.
- "Altair: definition of Altair in Oxford dictionary (American English)".
- 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
- Ducati, J. R. (2002). "VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system". CDS/ADC Collection of Electronic Catalogues. 2237: 0. Bibcode:2002yCat.2237....0D.
- NAME ALTAIR -- Variable Star of delta Sct type, database entry, SIMBAD. Accessed on line November 25, 2008.
- Buzasi, D. L.; Bruntt, H.; Bedding, T. R.; Retter, A.; Kjeldsen, H.; Preston, H. L.; Mandeville, W. J.; Suarez, J. C.; Catanzarite, J. (February 2005). "Altair: The Brightest δ Scuti Star". The Astrophysical Journal. 619 (2): 1072–1076. arXiv:astro-ph/0405127. Bibcode:2005ApJ...619.1072B. doi:10.1086/426704. ISSN 0004-637X. S2CID 16524681.
- Monnier, J. D.; Zhao, M; Pedretti, E; Thureau, N; Ireland, M; Muirhead, P; Berger, J. P.; Millan-Gabet, R; Van Belle, G; Ten Brummelaar, T; McAlister, H; Ridgway, S; Turner, N; Sturmann, L; Sturmann, J; Berger, D (2007). "Imaging the surface of Altair". Science. 317 (5836): 342–345. arXiv:0706.0867. Bibcode:2007Sci...317..342M. doi:10.1126/science.1143205. PMID 17540860. S2CID 4615273. See second column of Table 1 for stellar parameters.CS1 maint: postscript (link)
- Peterson, D. M.; Hummel, C. A.; Pauls, T. A.; et al. (2006). "Resolving the Effects of Rotation in Altair with Long‐Baseline Interferometry". The Astrophysical Journal. 636 (2): 1087–1097. arXiv:astro-ph/0509236. Bibcode:2006ApJ...636.1087P. doi:10.1086/497981. S2CID 18683397. See Table 2 for stellar parameters.
- Malagnini, M. L.; Morossi, C. (November 1990), "Accurate absolute luminosities, effective temperatures, radii, masses and surface gravities for a selected sample of field stars", Astronomy and Astrophysics Supplement Series, 85 (3): 1015–1019, Bibcode:1990A&AS...85.1015M
- Robrade, J.; Schmitt, J. H. M. M. (April 2009), "Altair - the "hottest" magnetically active star in X-rays", Astronomy and Astrophysics, 497 (2): 511–520, arXiv:0903.0966, Bibcode:2009A&A...497..511R, doi:10.1051/0004-6361/200811348, S2CID 14320453.
- HR 7557, 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 November 25, 2008.
- Entry 19508+0852, The Washington Double Star Catalog Archived 2009-01-31 at the Wayback Machine, United States Naval Observatory. Accessed on line November 25, 2008.
- Kunitzsch, Paul; Smart, Tim (2006). A Dictionary of Modern star Names: A Short Guide to 254 Star Names and Their Derivations (2nd rev. ed.). Cambridge, Massachusetts: Sky Pub. ISBN 978-1-931559-44-7.
- "Our Local Galactic Neighborhood". NASA. Archived from the original on 2013-11-21.
- Gilster, Paul (2010-09-01). "Into the Interstellar Void". Centauri Dreams. Retrieved 2017-03-26.
- Altair, entry, The Internet Encyclopedia of Science, David Darling. Accessed on line November 25, 2008.
- Summer Triangle, entry, The Internet Encyclopedia of Science, David Darling. Accessed on line November 26, 2008.
- Hoboken, Fred Schaaf (2008). The brightest stars : discovering the universe through the sky's most brilliant stars. New Jersey: John Wiley & Sons, Inc. p. 194. ISBN 978-0-471-70410-2. OCLC 440257051.
- Belle, Gerard T. van; Ciardi, David R.; Thompson, Robert R.; Akeson, Rachel L.; Lada, Elizabeth A. (2001). "Altair's Oblateness and Rotation Velocity from Long-Baseline Interferometry". The Astrophysical Journal. 559 (2): 1155–1164. Bibcode:2001ApJ...559.1155V. doi:10.1086/322340. ISSN 0004-637X.
- "the definition of altair". www.dictionary.com. Retrieved 2018-09-30.
- "IAU Working Group on Star Names (WGSN)". Retrieved 22 May 2016.
- "Bulletin of the IAU Working Group on Star Names, No. 1" (PDF). Retrieved 28 July 2016.
- "IAU Catalog of Star Names". Retrieved 28 July 2016.
- p. 190, Schaaf 2008.
- The stellar interferometer at Narrabri Observatory-II. The angular diameters of 15 stars, R. Hanbury Brown, J. Davis, L. R. Allen, and J. M. Rome, Monthly Notices of the Royal Astronomical Society 137 (1967), pp. 393–417, Bibcode:1967MNRAS.137..393H.
- Ohishi, Naoko; Nordgren, Tyler E.; Hutter, Donald J. (2004). "Asymmetric Surface Brightness Distribution of Altair Observed with the Navy Prototype Optical Interferometer". The Astrophysical Journal. 612 (1): 463–471. arXiv:astro-ph/0405301. Bibcode:2004ApJ...612..463O. doi:10.1086/422422. S2CID 15857535.
- Domiciano de Souza, A.; Kervella, P.; Jankov, S.; Vakili, F.; Ohishi, N.; Nordgren, T. E.; Abe, L. (2005). "Gravitational-darkening of Altair from interferometry". Astronomy & Astrophysics. 442 (2): 567–578. Bibcode:2005A&A...442..567D. doi:10.1051/0004-6361:20042476.
- Gazing up at the Man in the Star?, Press Release 07-062, National Science Foundation, May 31, 2007. Accessed on line November 25, 2008.
- Knobel, E. B. (June 1895). "Al Achsasi Al Mouakket, on a catalogue of stars in the Calendarium of Mohammad Al Achsasi Al Mouakket". Monthly Notices of the Royal Astronomical Society. 55 (8): 429–438. Bibcode:1895MNRAS..55..429K. doi:10.1093/mnras/55.8.429.
- pp. 17–18, A Dictionary of Modern Star Names, Paul Kunitzsch and Tim Smart, Cambridge, Massachusetts: Sky Publishing, 2006, ISBN 978-1-931559-44-7.
- p. 59–60, Star-names and Their Meanings, Richard Hinckley Allen, New York: G. E. Stechert, 1899.
- Gingerich, O. (1987). "Zoomorphic Astrolabes and the Introduction of Arabic Star Names into Europe". Annals of the New York Academy of Sciences. 500 (1): 89–104. Bibcode:1987NYASA.500...89G. doi:10.1111/j.1749-6632.1987.tb37197.x. S2CID 84102853.
- p. 4, Aboriginal mythology : an A-Z spanning the history of aboriginal mythology from the earliest legends to the present day, Mudrooroo, London: HarperCollins, 1994, ISBN 1-85538-306-3.
- p. 115, Mudrooroo 1994.
- (in Chinese) 香港太空館 - 研究資源 - 亮星中英對照表 Archived 2008-10-25 at the Wayback Machine, Hong Kong Space Museum. Accessed on line November 26, 2008.
- pp. 97–98, 161, The Chinese Reader's Manual, William Frederick Mayers, Shanghai: American Presbyterian Mission Press, 1874.
- p. 72, China, Japan, Korea Culture and Customs: Culture and Customs, Ju Brown and John Brown, 2006, ISBN 978-1-4196-4893-9.
- pp. 105–107, Magic Lotus Lantern and Other Tales from the Han Chinese, Haiwang Yuan and Michael Ann Williams, Libraries Unlimited, 2006, ISBN 978-1-59158-294-6.
- p. 175, The Lexicon of Proto Oceanic: The Culture and Environment of Ancestral Oceanic Society: The Physical Environment, Volume 2, Malcolm Ross, Andrew Pawley and Meredith Osmond, Canberra, The Australian National University E Press, 2007.
- Kelley, David H.; Milone, Eugene F.; Aveni, A.F. (2011). Exploring Ancient Skies: A Survey of Ancient and Cultural Astronomy. New York, New York: Springer. p. 344. ISBN 978-1-4419-7623-9.
- NASA names next-gen lunar lander Altair, December 13, 2007, collectspace.com. Accessed on line November 26, 2008.
- Press release #58, Beriev Aircraft Company, February 12, 2003. Accessed on line November 26, 2008.
- 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.
- BD+08 4236B -- Star in double system, database entry, SIMBAD. Accessed on line November 25, 2008.
- BD+08 4238 -- Star in double system, database entry, SIMBAD. Accessed on line November 25, 2008.
|Wikimedia Commons has media related to Altair.|
- Star with Midriff Bulge Eyed by Astronomers, JPL press release, July 25, 2001.
- Imaging the Surface of Altair, University of Michigan news release detailing the CHARA array direct imaging of the stellar surface in 2007.
- PIA04204: Altair, NASA. Image of Altair from the Palomar Testbed Interferometer.
- Altair, SolStation.
- Secrets of Sun-like star probed, BBC News, June 1, 2007.
- Astronomers Capture First Images of the Surface Features of Altair, Astromart.com
- Image of Altair from Aladin.