Chi Aurigae

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Template:Short description Template:Sky

Chi Aurigae
Template:Location mark
The location of χ Aurigae (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Auriga
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) 4.74[2]
Characteristics
Spectral type B5 Iab[3]
U−B Template:Engvar −0.44[2]
B−V Template:Engvar +0.32[2]
Astrometry
Radial velocity (Rv)7.27±5.21[1] km/s
Proper motion (μ) RA: −0.812 mas/yr[1]
Dec.: −3.15 mas/yr[1]
Parallax (π)0.9087±0.1906 mas[1]
DistanceScript error: No such module "val". ly
(Script error: No such module "val". pc)[4]
Absolute magnitude (MV)−6.4[5]
Orbit[5]
Period (P)676.85 ± 0.21 d
Eccentricity (e)0.116 ± 0.048
Longitude of the node (Ω)181.7° ± 24.3°
Periastron epoch (T)2422754.2 ± 46.1 HJD
Semi-amplitude (K1)
(primary)
22.0 ± 2.9 km/s
Details
MassScript error: No such module "val".[4] Template:Solar mass
RadiusScript error: No such module "val".[4] Template:Solar radius
LuminosityScript error: No such module "val".[4] Template:Solar luminosity
Surface gravity (log g)Script error: No such module "val".[4] cgs
TemperatureScript error: No such module "val".[4] K
Rotational velocity (v sin i)40[6] km/s
Age8.7[4] Myr
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[7]
Database references
SIMBADdata

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Chi Aurigae is a binary star system in the northern constellation of Auriga. Its name is a Bayer designation that is Latinized from χ Aurigae, and abbreviated Chi Aur or χ Aur. This star is visible to the naked eye with an apparent visual magnitude of 4.74.[2] The brightness of the star is diminished by 1.26 in magnitude from extinction caused by intervening gas and dust.[5] It is a member of the Aur OB1 association of co-moving stars.[5]

Chi Aurigae is a single-lined spectroscopic binary with an orbital period of 676.85 d and an eccentricity of 0.116.[5] The primary component of this system is a supergiant star with a stellar classification of B5 Iab.[3] It is over 190,000 times more luminous, around 20 times more massive and around 70 times larger than the Sun. The photosphere has an effective temperature of 14,600 K.[4] Its stellar wind is causing mass loss at the rate of Script error: No such module "val". solar masses per year, or the equivalent of the Sun's mass every 2.4 billion years.[8]

The distance of Chi Aurigae is determined at 3,900 light-years based on spectroscopic observations.[4] Parallax measurements by the Hipparcos spacecraft were unsuccessful because the parallax error was bigger than the value itself,[9] while the Gaia spacecraft measured the parallax with a 22% error, giving a distance of Script error: No such module "val"..[1]

References

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  1. a b c d e f Template:Cite DR3
  2. a b c d Script error: No such module "citation/CS1".
  3. a b Script error: No such module "citation/CS1".
  4. a b c d e f g h i Script error: No such module "citation/CS1".
  5. a b c d e Script error: No such module "citation/CS1".
  6. Script error: No such module "citation/CS1".
  7. Template:Cite simbad
  8. Script error: No such module "citation/CS1".
  9. Script error: No such module "citation/CS1". Note: see VizieR catalogue I/311.

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External links

Template:Stars of Auriga