HD 172167 (Vega)
Spectral type: A0 V

VEGA (Alpha Lyra) is one of the most famed stars of the sky. At magnitude zero, it is the sky's fifth brightest star, falling just behind Arcturus and just ahead of Capella. It is also one of the closer stars to the Earth, lying just 25 light years away. Though its proximity helps make it bright in our skies, it is also inherently luminous, some 50 times brighter than our Sun. Vega is a classic main sequence star, like the Sun quietly running off the nuclear fusion of hydrogen deep in its core. Its color and apparent brightness made it the basic standard against which the apparent magnitudes of all other stars are ultimately compared.

Vega was one of the first stars to be discovered with a large luminous infrared-radiating halo that suggests a circumstellar cloud of warm dust. Since Vega seems to be rotating with its pole directed toward the Earth, the dust cloud probably represents a face-on disk that may not be unlike the disk surrounding the Sun and that contains the planets. Several other stars similar to Vega (Beta Pic and Fomalhault for example) possess similar disks.


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