HR 5553
Observation data Epoch J2000 Equinox J2000 | ||
---|---|---|
Constellation | Boötes | |
Right ascension | 14h 53m 23.76674s[2] | |
Declination | +19° 09′ 10.0813″[2] | |
Apparent magnitude (V) | 6.00[3] (5.97 to 6.04)[4] | |
Characteristics | ||
Spectral type | K0 V[5] | |
U−B color index | +0.49[5] | |
B−V color index | +0.84[5] | |
Variable type | RS CVn[4] | |
Absolute magnitude (MV) | 5.69[7] | |
Argument of periastron (ω)(secondary) | 219±0.1° | |
Details | ||
HR 5553 A | ||
Gyr | ||
HR 5553 B | ||
Mass | 0.45[5] M☉ | |
LHS 5279[12] | ||
Database references | ||
SIMBAD | data |
HR 5553 is a
apparent visual magnitude from 5.97 down to 6.04,[4] which is bright enough to be dimly visible to the naked eye. The system is drifting closer to the Sun with a radial velocity of −30 km/s,[6] and is expected to come as close as 26.9 light-years in 210,000 years.[13]
Orbital elements for this single-lined
spectroscopic binary was first calculated in 1981 using radial velocity measurements from David Dunlap Observatory combined with older measurements from Mount Wilson Observatory and Dominion Astrophysical Observatory.[14] The two stars orbit each other with a period of 125 days and a large eccentricity of 0.51.[5]
The primary, designated component A, is a
luminosity of the Sun from its photosphere at an effective temperature of 5,313 K.[10] Component B has an estimated 45% of the mass of the Sun.[5]
An
AU. The temperature of this dust is 40 K.[10] The estimated mass of the dust is 0.0002 times the mass of the Earth. It is aligned to within 10° of the plane of the binary system.[9][8]
References
- doi:10.1086/117740. Retrieved 5 November 2021.
- ^ S2CID 18759600.
- Bibcode:1986EgUBV........0M.
- ^ S2CID 125853869.
- ^ S2CID 53686506.
- ^ S2CID 15290475.
- S2CID 118577511.
- ^ .
- ^ S2CID 119232172, A114.
- ^ S2CID 377244.
- ^ S2CID 27151456.
- ^ "DE Boo". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-12-07.
- S2CID 56269929.
- Bibcode:1981JRASC..75...56K.