Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Ara |
Right ascension | 17h 01m 47.3875s [2] |
Declination | –58° 57′ 29.681″ [2] |
Apparent magnitude (V) | 6.137 [3] |
Characteristics | |
Spectral type | B1 V:ne [4] or B2 IVne [5] |
U−B color index | –0.956 [3] |
B−V color index | –0.078 [3] |
Astrometry | |
Radial velocity (Rv) | –6 [6] km/s |
Proper motion (μ) |
RA: –2.91
[2]
mas/
yr Dec.: –9.01 [2] mas/ yr |
Parallax (π) | 2.32 ± 0.38 mas [2] |
Distance | approx. 1,400
ly (approx. 430 pc) |
Details | |
Mass | 10.1 ± 0.3 [5] M☉ |
Radius | 4.5 [7] R☉ |
Luminosity (bolometric) | 11,045 [8] L☉ |
Temperature | 21,150 [8] K |
Age | 20.4 ± 0.4 [5] Myr |
Other designations | |
Database references | |
SIMBAD | data |
HD 153261 is the Henry Draper Catalogue designation for a star in the southern constellation of Ara. It has an apparent visual magnitude of 6.137, [3] placing it near the threshold of naked eye visibility. According to the Bortle Dark-Sky Scale, it can be viewed from dark suburban or rural skies. Based upon an annual parallax shift of just 2.32 mas, [2] it is located at a distance of around 1,400 light-years (430 parsecs) from Earth.
This star has been catalogued with a stellar classification of B1 V:ne [4] or B2 IVne, [5] indicating that it is either a main sequence or a subgiant star. The 'n' indicates a nebulous spectrum created by the Doppler shift-broadened absorption lines from a rapid rotation, while the 'e' means this is a Be star, with the spectrum showing emission lines from hot, circumstellar gas. HD 153261 displays some variability with an amplitude of 0.090 in magnitude, and is a suspected spectroscopic binary. [1]
HD 153261 is a large star with over ten [5] times the Sun's mass and around 4.5 [7] the radius of the Sun. It shines with more than 11,000 [8] times the brightness of the Sun, with this energy being radiated into space at an effective temperature of 21,150 K. [8] At this heat, it glows with the blue-white hue of a B-type star. [10]
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