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Vega

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Wikipedia-Article "Vega"

This article is about Vega, the star. For other uses: see Vega (disambiguation)
Vega
Observation data
Epoch J2000
Constellation Lyra
Right ascension 18h 36m 56.3s
Declination +38° 47' 01"
Apparent magnitude (V) 0.03
Characteristics
Spectral type A0 V
B-V color index 0.00
U-B color index -0.01
Variable type Delta Scuti
Astrometry
Radial velocity (Rv) -13.5 km/s
Proper motion (μ) RA: 201.02 mas/yr
Dec.: 287.46 mas/yr
Parallax (π) 129.01 ± 0.52 mas
Distance 25.27 ly (7.751 pc)
Absolute magnitude (MV) 0.58
Details
Mass 2.6 M
Radius 3.1 R
Luminosity 51 L
Temperature 9,300 K
Metallicity 63%
Rotation  ?
Age 3.5 × 108 years
Other designations
Alpha Lyra, α Lyra, 3 Lyr, GJ 721, HR 7001, BD +38°3238, HD 91262, GCTP 4293.00, LTT 15486, SAO 67174, HIP 91262.

Vega (α Lyr / α Lyrae / Alpha Lyrae) is the brightest star in the constellation Lyra, and the fifth brightest star in the sky. It is the second brightest star in the Northern night sky, after Arcturus, and can often be seen near the zenith in the mid-northern latitudes during the Northern Hemisphere summer.

It is a "nearby star" at only 25.3 light years (148.6 trillion miles) from Earth, and together with Arcturus and Sirius, one of the brightest stars in the Sun's neighbourhood.

Vega is a vertex of the Summer Triangle, which consists of Vega (in Lyra), Deneb (in Cygnus) and Altair (in Aquila). If one is to consider this asterism a right triangle, then Vega would correspond to its right angle. This triangle is very recognisable in the northern skies for there are few bright stars in its vicinity.

Its spectral class is A0V (Sirius, an A1V, is slightly less powerful) and it is firmly in the main sequence, fusing hydrogen to helium in its core. Since more powerful stars use their fusion fuel more quickly than smaller ones, Vega's life time is only one billion years, a tenth of our Sun's. Vega is two and a half times more massive than our Sun and burns at fifty times the power.

In about AD 14,000, Vega will become the North Star, owing to the precession of the equinoxes. See Polaris for more information.

Professional astronomers have used Vega for the calibration of absolute photometric brightness scales. When the magnitude scale was fixed, Vega happened to be close to zero magnitude. Therefore the visual magnitude of Vega was decided to be, by definition, zero at all wavelengths (this is no longer the case, as apparent magnitude is now most commonly defined in terms of the flux from the star). It also has a relatively flat electromagnetic spectrum in the visual region (wavelength range 350-850 nanometers, most of which can be seen with the human eye), so the flux densities are roughly equal, 2000-4000 Jy. The flux density of Vega drops rapidly in the infrared, and is near 100 Jy at 5 micrometres.

The name Vega comes from the Arabic word waqi meaning "falling", via the phrase نسر الواقع an-nasr al-wāqi‘, translated "the swooping vulture". As part of the constellation Lyra it represents a jewel set in the body of the harp.

Contents

Possible planetary system

Vega has a disk of dust and gas around it, discovered by the IRAS satellite in the mid 1980s. This was initially thought to be a protoplanetary disk, but is now considered a "debris disk" due to the star's relatively young age of about 200 million years. In 1998 teams at the Joint Astronomy Centre and UCLA detected irregularities in it that suggest the presence of a planet.[1] A 2003 paper hypothesizes these lumps could be caused by a Neptune-sized planet having migrated from 40 to 65 AU over 56 million years[2], an orbit large enough to allow the formation of smaller rocky planets closer to Vega.[3] These findings have yet to be fully confirmed, but since Vega is much more powerful than our Sun, scientists believe there is no life possible on any such suggested planets.

Cultural significance

The star has been the subject of many 'firsts' in Astronomy; in 1850 it became the first star to be photographed, and in 1872 the first to have its spectrum photographed. It was also debatably the first star to have its parallax measured, in the pioneering experiments of Friedrich Struve in 1837. Finally, it became the first star to have a car named after it, when Chevrolet launched the 'Vega' in 1971.

In Chinese mythology, there is a love story of Qi Xi 七夕 in which Niu Lang 牛郎 (Altair) and his two children (β and γ Aquilae) are separated forever from their mother Zhi Nü 織女(Vega) who is on the far side of the river, the Milky Way 銀河. The Japanese Tanabata festival is also based on this legend.

In Hindu astronomy, Vega is called Abhijit.

Medieval astrologers counted Vega one of the Behenian stars and related it to chrysolite and winter savory. Cornelius Agrippa listed its kabbalistic sign Image:Agrippa1531_Vulturcadens.png under Vultur cadens, a literal Latin translation of the Arabic name.

Science fiction

Alternative and former names

  • "The Falling Eagle"
  • "The Harp Star"
  • Wega (a closer transliteration of the Arabic)
  • Akkadian: Tir-anna, "Life of Heaven"
  • Babylonian: Dilgan, "the Messenger of Light"
  • Chinese: Zhi Nü, "the Weaver"
  • Greek: Allore
  • Sanskrit: Abhijit, "Victorious"
  • Latin: Fidis, "Lyre"; Vultur cadens, "Falling vulture"

Alternative catalogue names include 3 Lyrae (Flamsteed); HD 172167; HR 7001

References

External links

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