Beta Arae

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Template:Short description

β Arae
Template:Location mark
Location of β Arae (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Ara
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) 2.84[2]
Characteristics
Evolutionary stage Red supergiant
Spectral type K0/1Ib[3]
U−B Template:Engvar +1.56[4]
B−V Template:Engvar +1.46[4]
Astrometry
Radial velocity (Rv)Template:Val[5] km/s
Proper motion (μ) RA: Template:Val mas/yr[6]
Dec.: Template:Val mas/yr[6]
Parallax (π)4.5601±0.2077 mas[1]
DistanceTemplate:Val ly
(Template:Val pc)[7]
Absolute magnitude (MV)−3.494[8]
Details[9]
MassTemplate:Val or 7.89±0.4 Template:Solar mass
RadiusTemplate:Val Template:Solar radius
LuminosityTemplate:Val Template:Solar luminosity
Surface gravity (log g)Template:Val cgs
TemperatureTemplate:Val K
Metallicity [Fe/H]Template:Val dex
Rotational velocity (v sin i)Template:Val[5] km/s
AgeTemplate:Val[10] Myr
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[11]
Database references
SIMBADdata

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Beta Arae is the brightest star in the constellation of Ara. This is a very luminous, relatively young red supergiant with an apparent visual magnitude of 2.84 and an absolute magnitude of −3.494.[2][8] Its name is a Bayer designation that is Latinized from β Arae, and abbreviated Beta Ara or β Ara. Based on a photogeometric estimation method, it is 710 light-years away,[7] a distance of which interstellar extinction in the line of sight reduces its apparent magnitude by 0.193 magnitudes.[9]

Characteristics

The spectrum of this star matches a stellar classification of K0/1 Ib,[3] with the luminosity class notation 'Ib' indicating that the star is a supergiant. It has an age estimated at 50 million years,[10] having spent much of its life as a B-type star.[12] Currently, it has expanded to 141 times the Sun's size and is 5,800 times more luminous.[9] Beta Arae is radiating energy from its outer envelope at an effective temperature of Template:Val, which causes it to take on the orange hue of a K-type star.[13] This enlarged star appears to be rotating slowly with a projected rotational velocity of about Template:Val.[5] The abundance of elements other than hydrogen and helium, its metallicity, is more than three times that of the Sun.[5]Template:Efn

Nomenclature

Beta Arae is the star's Bayer designation. Other designations include HD 157244 (from the Henry Draper Catalogue), HIP 85258 (from the Hipparcos catalogue) and HR 6461 (from the Bright Star Catalogue).[11]

Rarely, this star is called Vasat-ül-cemre a Turkisation of Arabic وسط الجمر (wasaṭ al-jamar), meaning "middle of the embers."[14] The constellation is named in Arabic المجمرة (al-mijmarah), meaning brazier/incense-burner.[15] In Chinese, Script error: No such module "Lang". (Script error: No such module "Lang".), meaning Pestle, refers to an asterism of β, σ and α Arae.[16] The Chinese name for β Arae is Script error: No such module "Lang". (Script error: No such module "Lang"., Template:Langx.)[17]

Notes

Template:Notelist

References

Template:Reflist

External links

Template:Stars of Ara Template:Portal bar

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