Rho1 Arae
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Ara |
| Right ascension | 16h 56m 08.8420s |
| Declination | −50° 40′ 29.243″ |
| Apparent magnitude (V) | 6.275 |
| Characteristics | |
| Spectral type | B3 Vnpe |
| U−B color index | −0.691 |
| B−V color index | +0.008 |
| Variable type | Be star |
| Astrometry | |
| Radial velocity (Rv) | +19.0±4.3 km/s |
| Proper motion (μ) | RA: −9.403 mas/yr Dec.: −9.592 mas/yr |
| Parallax (π) | 3.3089±0.0441 mas |
| Distance | 990 ± 10 ly (302 ± 4 pc) |
| Absolute magnitude (MV) | −0.16 |
| Orbit | |
| Period (P) | 236.50±0.18 d |
| Inclination (i) | 60±7° |
| Periastron epoch (T) | 2458672.10±0.72 HJD |
| Semi-amplitude (K1) (primary) | 4.33±0.05 km/s |
| Semi-amplitude (K2) (secondary) | 52.83±1.49 km/s |
| Details | |
| ρ1 Ara A | |
| Mass | 6.5±1.3 M☉ |
| Radius | 4.21±0.20 R☉ |
| Luminosity | 1,418 L☉ |
| Surface gravity (log g) | 3.75 cgs |
| Temperature | 19,800 K |
| Rotational velocity (v sin i) | 370±10 km/s |
| Age | 18.4±1.5 Myr |
| ρ1 Ara B | |
| Mass | 0.53±0.11 M☉ |
| Radius | 0.27±0.04 R☉ |
| Luminosity | 204 L☉ |
| Temperature | 42,000 K |
| Other designations | |
| ρ1 Ara, V846 Arae, NSV 8047, CD−50 10905, GC 22790, HD 152478, HIP 82868, HR 6274, SAO 244280, PPM 345531 | |
| Database references | |
| SIMBAD | data |
Rho1 Arae is a star in the southern constellation of Ara. Its name is a Bayer designation that is Latinized from ρ1 Arae, and abbreviated Rho1 Ara or ρ1 Ara. Unusually for a star with a Bayer designation, it was not catalogued by Bayer in his Uranometria. It was instead first catalogued by Nicolas Lacaille, in his Coelum Australe Stelliferum published in 1763. This star gained the designation of Rho1 Arae in Bode's Uranographia, published in 1801. Rho1 Arae is one of the dimmest stars with a Bayer designation, having an apparent visual magnitude of just +6.275. According to the Bortle Dark-Sky Scale, this means the star is just barely visible to the naked eye in dark rural skies. Based upon parallax measurements, it is about 990 light-years (302 parsecs) distant from the Sun. It is receding from the Sun with a radial velocity of +19 km/s.
Hipparcos data revealed that Rho1 Arae is a variable star. It was given its variable star designation, V846 Arae, in 1999. This is a spectroscopic binary system, which means that the presence of an orbiting companion is indicated by shifts in the spectrum. The primary star is a Be star, while the secondary star is a subdwarf O star; they orbit each other with a period of about 236.50 days.
The combined spectrum of this system matches a stellar classification of B3 Vnpe, which may indicate the primary is a B-type main-sequence star. The 'e' suffix indicates the presence of emission lines from the primary Be star. The primary star is spinning rapidly with a projected rotational velocity of 370±10 km/s, which makes it difficult to obtain reliable orbital elements. For Rho1 Arae, the emission lines are prominent and variable. The observed variability may be the result of a magnetized stellar wind that is flowing close to the circumstellar disk.
Rho1 Arae has a peculiar velocity of 27.4±4.9 km/s relative to its neighbors, making it a runaway star system. A scenario that it was ejected from the Scorpius–Centaurus OB association as a result of a past supernova explosion seems unlikely because of its binarity.