52 Sagittarii
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Sagittarius |
Right ascension | 19h 36m 42.43288s[1] |
Declination | −24° 53′ 01.0288″[1] |
Apparent magnitude (V) | 4.59[2] + 9.2 |
Characteristics | |
Evolutionary stage | main sequence[3] |
Spectral type | B8/9V[4] + K2–4V |
U−B color index | −0.15[5] |
B−V color index | −0.06[5] |
Absolute magnitude (MV) | 0.77[2] |
Details | |
52 Sgr A | |
Myr | |
Database references | |
SIMBAD | data |
52 Sagittarii is a
apparent visual magnitude of 4.59.[2] It is located approximately 190 light years away based on parallax,[1] but is drifting closer with a radial velocity of −19 km/s.[6]
The primary component is a
projected rotational velocity of 48 km/s.[3]
52 Sagittarii has one companion at an
″. This object is magnitude 9.2 with a spectral class in the K2V-K4V range, and is believed to be the source of X-ray emissions from the system.[14][15]
References
- ^ S2CID 18759600. Vizier catalog entry
- ^ S2CID 119257644. Vizier catalog entry
- ^ S2CID 55586789. Vizier catalog entry
- ^ Bibcode:1988mcts.book.....H.
- ^
- ^ LCCN 54001336.
- ^ S2CID 118629873. Vizier catalog entry
- ^ Bibcode:1999A&A...352..555A. Vizier catalog entry
- S2CID 33401607. Vizier catalog entry
- S2CID 118345778. Vizier catalog entry
- ^ "h02 Sgr". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-07-27.
- S2CID 14878976.
- doi:10.1086/116967. Garrison has note: "Balmer shell cores?"
- S2CID 15143368.