Altair

Altair, also called α Aquilae, α Aql, is the brightest star in the constellation of Aquila.

It is the twelfth brightest star in the night sky. It is in the G-cloud—a fog of gas and dust known as an interstellar cloud.^[1]^[2] Altair is an A-type main sequence star with an apparent visual magnitude of 0.77. It is one of the vertices of the Summer Triangle (the other two vertices are Deneb and Vega).^[3] It is 16.7 light-years (5.13 parsecs) from the Sun and is one of the closest stars visible to the naked eye.^[4]

Altair spins rapidly, with a velocity at its equator of about 286 km/s.^[5]^[6] This is a significant fraction of the star's estimated breakup speed of 400 km/s.^[7] A study with the Palomar Testbed Interferometer showed that Altair is not spherical, but is flattened at the poles due to its high rate of rotation.^[8] Other interferometric studies with multiple telescopes, operating in the infrared, have confirmed this.^[6]

References[change | change source]

↑ "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.
↑ 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. pp. 194. ISBN 978-0-471-70410-2. OCLC 440257051.
↑ From values of v sin i and i in the second column of Table 1, Monnier et al. 2007.
↑ ^6.0 ^6.1 Monnier J D.; et al. (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.
↑ Robrade J. & Schmitt J.H.M.M. 2009. Altair - the "hottest" magnetically active star in X-rays. Astronomy and Astrophysics, 497 (2): 511–520
↑ Belle, Gerard T. van; et al. (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. S2CID 13969695.^{[permanent dead link]}

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[1] "Our Local Galactic Neighborhood". NASA. Archived from the original on 2013-11-21.

[2] Gilster, Paul (2010-09-01). "Into the Interstellar Void". Centauri Dreams. Retrieved 2017-03-26.

[darlingsummer-3] Summer Triangle, entry, The Internet Encyclopedia of Science, David Darling. Accessed on line November 26, 2008.

[4] Hoboken, Fred Schaaf (2008). The brightest stars : discovering the universe through the sky's most brilliant stars. New Jersey: John Wiley & Sons, Inc. pp. 194. ISBN 978-0-471-70410-2. OCLC 440257051.

[5] From values of v sin i and i in the second column of Table 1, Monnier et al. 2007.

[monnier07-6] 6.0 ^6.1 Monnier J D.; et al. (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.

[7] Robrade J. & Schmitt J.H.M.M. 2009. Altair - the "hottest" magnetically active star in X-rays. Astronomy and Astrophysics, 497 (2): 511–520

[pti2001-8] Belle, Gerard T. van; et al. (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. S2CID 13969695.^{[permanent dead link]}

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