Beta Arae

Beta Arae (β Ara, β Arae), the brightest star in the constellation of Ara, is a very luminous, relatively young, giant star with an apparent visual magnitude of 2.8 (rounded). Parallax measurements place it at roughly 650 light-years (200 parsecs) from Earth.

β Arae
Location of β Arae (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Ara
Right ascension 17h 25m 17.98835s
Declination −55° 31 47.5868
Apparent magnitude (V) 2.84
Characteristics
Spectral type K3 Ib-II
U−B color index +1.56
B−V color index +1.46
Astrometry
Radial velocity (Rv)−0.30±0.20 km/s
Proper motion (μ) RA: −8.51 mas/yr
Dec.: −25.24 mas/yr
Parallax (π)4.5601 ± 0.2077 mas
Distance720 ± 30 ly
(219 ± 10 pc)
Absolute magnitude (MV)−3.494
Details
Mass8.21 ,6.2~7.3 M
Radius142; 92 R
Luminosity5,636 L
Surface gravity (log g)1.20 cgs
Temperature4,197 K
Metallicity [Fe/H]−0.05 dex
Rotational velocity (v sin i)5.4±1.0 km/s
Age50.1±4.4 Myr
Other designations
CPD55°8100, FK5 645, HD 157244, HIP 85258, HR 6461, SAO 244725
Database references
SIMBADdata

The spectrum of this star matches a stellar classification of K3 Ib-IIa, with the luminosity class notation 'Ib-IIa' indicating that the star lies part way between a higher luminosity bright giant (IIa) and a lower luminosity supergiant (Ib). This represents two of the evolutionary stages that a massive star passes through after it has exhausted the hydrogen at its core. Beta Arae is radiating energy from its outer envelope at an effective temperature of 4,200 K, which causes it to take on the orange hue of a K-type star. This enlarged star appears to be rotating slowly with a projected rotational velocity of about 5 km/s. The abundance of elements other than hydrogen and helium, its metallicity, is more than three times that of the Sun.

Rarely, this star is called Vasat-ül-cemre a Turkisation of Arabic وسط الجمر (wasaṭ al-jamar), meaning "middle of the embers." The constellation is named in Arabic المجمرة (al-mijmarah), meaning brazier/incense-burner. In Chinese, (Chǔ), meaning Pestle, refers to an asterism of β, σ and α Arae. The Chinese name for β Arae is 杵三 (Chǔ sān, English: the Third Star of Pestle.)

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