Véga

3Alp Lyr

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Vega — Alpha Lyrae, the leading star of the small constellation Lyra — is a white A-type star whose B–V colour index of −0.001 is almost exactly neutral, long making it a photometric benchmark for stellar colour. It shines at apparent magnitude 0.03 from a distance of 25 light-years, and its absolute magnitude of 0.6 shows an intrinsic brightness only modestly above the value it presents to Earth. Positioned at a northern declination of +38°, Vega climbs high overhead from mid-northern latitudes and forms one apex of the Summer Triangle. Its brilliance and pure white light make it one of the most recognisable stars of the northern summer evening.

Propriétés physiques

Classe Spectrale A Class A — A-type (White)
Indice de couleur (B−V) -0,001

Observation

Magnitude Apparente +0.03
Magnitude Absolue 0,60
Distance 25.0 ly
Constellation Lyra

Position

Ascension droite 18h 36,94m
Déclinaison 38° 47,02′

Related Chemistry

Explore the chemical elements connected to Véga on our sister site ChemFYI.

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Frequently Asked Questions

What type of star is Véga?
Véga is a Class A — A-type (White) star.
How far is Véga from Earth?
Véga is approximately 25.0 light-years from Earth.
Can you see Véga with the naked eye?
With an apparent magnitude of 0.03, Véga is visible to the naked eye.
What constellation is Véga in?
Véga is located in the constellation Lyra.