Altair
Star
Facts
- Distance
- 16.5 light-years
- Spectral class
- A7 V
- Surface temperature
- from 6850 K at the equator to 8710 K at the poles
- Rotation
- 2.8 turns a day
- Flattening
- equator about 22% wider than the poles
Altair is a white main-sequence star of spectral class A7 V: it is the brightest star in the constellation Aquila, 16.5 light-years from Earth, and shines about 10 times more than the Sun. It is one of the three corners of the Summer Triangle, with Vega and Deneb.
It spins so fast, almost three turns a day, that it looks flattened. As a result its equator is cooler and darker than its poles, about 6600 °C against 8400: this is gravity darkening.
Sources
- van Altena, Lee and Hoffleit 1995, General Catalogue of Trigonometric Stellar Parallaxes, 4th Ed., Yale University Observatory
- Hoffleit and Warren 1991, Yale Bright Star Catalogue, 5th Revised Ed. (V magnitudes, positions and spectral classes)
- Monnier et al. 2007, Science 317, 342 (shape of Altair)
- NASA Night Sky Network, Summer Triangle Corner: Altair
- NASA APOD, Stars of a Summer Triangle (27 June 2015)