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Vega

File:Lyra_constellation_map.svg · Wikimedia Commons · See Wikimedia Commons

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Also known as Alpha Lyrae, α Lyrae, 3 Lyrae, Lucida Lyrae, α Lyr, HD 172167, alf Lyr, GJ 721

Vega is the brightest star in the northern constellation of Lyra. It has the Bayer designation α Lyrae, which is Latinised to Alpha Lyrae and abbreviated Alpha Lyr or α Lyr. This star is relatively close at only from the Sun, and one of the most luminous stars in the Sun's neighborhood, being intrinsically brighter than any star nearer to the sun. It is the fifth-brightest star in the night sky, and the second-brightest star in the northern celestial hemisphere, after Arcturus.

AI overview

Vega is the brightest star in the constellation Lyra and the fifth-brightest star visible from Earth, located relatively close to our Sun. It matters to astronomy because it is one of the most luminous stars nearby and has long served as an important reference point for studying stars and measuring celestial distances.

AI-generated from the Wikipedia summary — may contain errors.

Wikidata facts

Distance from Earth
7.67
Diameter
3590000
Radius
2.818
Mass
2.135
Image
Vega Spitzer.jpg
Show 17 more facts
Commons category
Vega
spectral class
A0Va
catalog code
UBV M 23118
parallax
0.11
apparent magnitude
0.129
effective temperature
9505
right ascension
66793
declination
2320.9
radial velocity
-12.9
absolute magnitude
0.582
luminosity
40.12
metallicity
-0.43
stellar rotational velocity
20.5
surface gravity
3000
age estimated by a dating method
455
right ascension component of proper motion
201.85
declination component of proper motion
285.46
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via Wikidata · CC0

~32 min read

Article

15 sections
Contents
  • Nomenclature
  • Observation
  • Observational history
  • Physical characteristics
  • Rotation
  • Element abundance
  • Kinematics
  • Possible planetary system
  • Infrared excess
  • Debris disks
  • Possible planets
  • Etymology and cultural significance
  • Notes
  • References
  • External links

Vega is the brightest star in the northern constellation of Lyra. It has the Bayer designation α Lyrae, which is Latinised to Alpha Lyrae and abbreviated Alpha Lyr or α Lyr. This star is relatively close at only from the Sun, and one of the most luminous stars in the Sun's neighborhood, being intrinsically brighter than any star nearer to the sun. It is the fifth-brightest star in the night sky, and the second-brightest star in the northern celestial hemisphere, after Arcturus.

Vega has been extensively studied by astronomers, leading it to be termed "arguably the next most important star in the sky after the Sun". Vega was the northern pole star around 12000 BCE and will be so again around the year 13724, when its declination will be , less than six degrees from the Pole. Vega was the first star other than the Sun to have its image and spectrum photographed. It was one of the first stars whose distance was estimated through parallax measurements. Vega has functioned as the baseline for calibrating the photometric brightness scale and was one of the stars used to define the zero point for the UBV photometric system.

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