Rho1 Arae
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Ara |
Right ascension | 16h 56m 08.8405s[1] |
Declination | –50° 40′ 29.244″[1] |
Apparent magnitude (V) | 6.275[2] |
Characteristics | |
Spectral type | B3 Vnpe |
U−B color index | –0.691[2] |
B−V color index | +0.008[2] |
Absolute magnitude (MV) | −0.16[4] |
Details | |
Myr | |
Database references | |
SIMBAD | data |
Rho1 Arae is 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 640 light-years (200 parsecs) distant from the Sun, give or take a 50-light-year margin of error.[1]
This is a
emission lines, indicating this is a Be star. For Rho1 Arae, the emission lines are prominent and variable.[8]
Rho1 Arae has 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.[8]
References
- ^ S2CID 18759600.
- ^ Bibcode:1985A&AS...61..387K.
- Bibcode:1967IAUS...30...57E.
- S2CID 119257644.
- ^ S2CID 118629873.
- S2CID 111387483.
- ^ S2CID 118362423.
- ^ .
- ^ "rho01 Ara". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2012-08-01.
{{cite web}}
: CS1 maint: postscript (link) - ^ "MAST: Barbara A. Mikulski Archive for Space Telescopes". Space Telescope Science Institute. Retrieved 8 December 2021.