Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Lupus |
Right ascension | 14h 58m 31.92536s [1] |
Declination | −43° 08′ 02.2699″ [1] |
Apparent magnitude (V) | 2.68 [2] |
Characteristics | |
Spectral type | B2 III [3] |
U−B color index | −0.902 [4] |
B−V color index | −0.226 [4] |
Variable type | β Cep [5] |
Astrometry | |
Radial velocity (Rv) | +0.1 ± 1.0 [3] km/s |
Proper motion (μ) |
RA: −35.78
[1]
mas/
yr Dec.: −39.83 [1] mas/ yr |
Parallax (π) | 8.52 ± 0.18 mas [1] |
Distance | 383 ± 8
ly (117 ± 2 pc) |
Absolute magnitude (MV) | −3.3 [6] |
Details | |
Mass | 8.8±0.2 [7] M☉ |
Radius | 6.6 [8] R☉ |
Luminosity | 10,000 [6] L☉ |
Surface gravity (log g) | 3.76 [6] cgs |
Temperature | 24,090 [9] K |
Metallicity [Fe/H] | −0.35±0.11 [5] dex |
Rotational velocity (v sin i) | 92 [3] km/s |
Age | 24.6±2.7 [7] Myr |
Other designations | |
Database references | |
SIMBAD | data |
Beta Lupi ( Latinized from β Lupi) or Kekouan ( /ˈkɛkwɑːn/), is a star in the southern constellation of Lupus. It has an apparent visual magnitude of 2.7, [2] making it readily visible to the naked eye. Based upon parallax measurements, this star is located at a distance of about 383 light-years (117 parsecs) from Earth. [2]
The stellar classification of B2 III indicates this is a giant star. [3] The effective temperature of the star's outer envelope is 24,090 K, [9] giving it the blue-white hue of a B-type star. [11] With an age of around 25 million years, [7] it is near the end of its hydrogen phase, where hydrogen is fused into the element helium, and transferring into a red supergiant star. At about 8.8 [7] solar masses, it may have enough mass to end its life as a Type II supernova, but there is the possibility of Beta Lupi becoming a white dwarf. [12]
This is a multi-period Beta Cephei variable with a dominant oscillation period of 0.232 days. [5] It is a proper motion member of the Upper Centaurus–Lupus sub-group in the Scorpius–Centaurus OB association, the nearest such co-moving association of massive stars to the Sun. [6] Beta Lupi has a high proper motion of more than 50 mas per year, suggesting a significant transverse velocity. [13]
It is positioned about 1.3° SSW of the supernova remnant SN 1006. [14]
In Chinese, 騎官 (Qí Guān), meaning Imperial Guards, refers to an asterism consisting of β Lupi, γ Lupi, δ Lupi, κ Centauri, λ Lupi, ε Lupi, μ Lup, π Lupi, ο Lupi and α Lupi. [15] Consequently, the Chinese name for β Lupi itself is 騎官四 (Qí Guān sì, English: the Fourth Star of Imperial Guards.). [16] From the French rendering of this Chinese name derives the traditional European name Kekouan (Ke Kwan). [17]
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Lupus |
Right ascension | 14h 58m 31.92536s [1] |
Declination | −43° 08′ 02.2699″ [1] |
Apparent magnitude (V) | 2.68 [2] |
Characteristics | |
Spectral type | B2 III [3] |
U−B color index | −0.902 [4] |
B−V color index | −0.226 [4] |
Variable type | β Cep [5] |
Astrometry | |
Radial velocity (Rv) | +0.1 ± 1.0 [3] km/s |
Proper motion (μ) |
RA: −35.78
[1]
mas/
yr Dec.: −39.83 [1] mas/ yr |
Parallax (π) | 8.52 ± 0.18 mas [1] |
Distance | 383 ± 8
ly (117 ± 2 pc) |
Absolute magnitude (MV) | −3.3 [6] |
Details | |
Mass | 8.8±0.2 [7] M☉ |
Radius | 6.6 [8] R☉ |
Luminosity | 10,000 [6] L☉ |
Surface gravity (log g) | 3.76 [6] cgs |
Temperature | 24,090 [9] K |
Metallicity [Fe/H] | −0.35±0.11 [5] dex |
Rotational velocity (v sin i) | 92 [3] km/s |
Age | 24.6±2.7 [7] Myr |
Other designations | |
Database references | |
SIMBAD | data |
Beta Lupi ( Latinized from β Lupi) or Kekouan ( /ˈkɛkwɑːn/), is a star in the southern constellation of Lupus. It has an apparent visual magnitude of 2.7, [2] making it readily visible to the naked eye. Based upon parallax measurements, this star is located at a distance of about 383 light-years (117 parsecs) from Earth. [2]
The stellar classification of B2 III indicates this is a giant star. [3] The effective temperature of the star's outer envelope is 24,090 K, [9] giving it the blue-white hue of a B-type star. [11] With an age of around 25 million years, [7] it is near the end of its hydrogen phase, where hydrogen is fused into the element helium, and transferring into a red supergiant star. At about 8.8 [7] solar masses, it may have enough mass to end its life as a Type II supernova, but there is the possibility of Beta Lupi becoming a white dwarf. [12]
This is a multi-period Beta Cephei variable with a dominant oscillation period of 0.232 days. [5] It is a proper motion member of the Upper Centaurus–Lupus sub-group in the Scorpius–Centaurus OB association, the nearest such co-moving association of massive stars to the Sun. [6] Beta Lupi has a high proper motion of more than 50 mas per year, suggesting a significant transverse velocity. [13]
It is positioned about 1.3° SSW of the supernova remnant SN 1006. [14]
In Chinese, 騎官 (Qí Guān), meaning Imperial Guards, refers to an asterism consisting of β Lupi, γ Lupi, δ Lupi, κ Centauri, λ Lupi, ε Lupi, μ Lup, π Lupi, ο Lupi and α Lupi. [15] Consequently, the Chinese name for β Lupi itself is 騎官四 (Qí Guān sì, English: the Fourth Star of Imperial Guards.). [16] From the French rendering of this Chinese name derives the traditional European name Kekouan (Ke Kwan). [17]