Observation data Epoch J2000.0 Equinox J2000.0 ( ICRS) | |
---|---|
Constellation | Sagittarius |
Right ascension | 20h 23m 53.17666s [1] |
Declination | −42° 25′ 22.3376″ [1] |
Apparent magnitude (V) | +5.64 [2] (6.04 + 7.12) [3] |
Characteristics | |
Spectral type | A5 V [4] (A1 + A6) [5] |
U−B color index | +0.099 [2] |
B−V color index | +0.192 [2] |
Astrometry | |
Radial velocity (Rv) | +2.6 [6] km/s |
Proper motion (μ) |
RA: −13.07
[1]
mas/
yr Dec.: +13.64 [1] mas/ yr |
Parallax (π) | 10.47 ± 0.50 mas [1] |
Distance | 310 ± 10
ly (96 ± 5 pc) |
Absolute magnitude (MV) | 1.03/2.35 [5] |
Orbit [7] | |
Period (P) | 700 yr |
Semi-major axis (a) | 2.032″ |
Eccentricity (e) | 0.401 |
Inclination (i) | 80° |
Longitude of the node (Ω) | 40.7° |
Periastron epoch (T) | 1912.00 |
Argument of periastron (ω) (secondary) | 177.3° |
Details | |
κ2 Sgr A | |
Mass | 1.85 [8] M☉ |
Luminosity | 38 [9] L☉ |
Surface gravity (log g) | 4.03 [8] cgs |
Temperature | 7,990±272 [8] K |
Age | 833 [8] Myr |
Other designations | |
Database references | |
SIMBAD | data |
Kappa2 Sagittarii (κ2 Sagittarii) is a binary star [3] system in the zodiac constellation of Sagittarius. It is visible to the naked eye with a combined apparent visual magnitude of +5.64. [2] Based upon an annual parallax shift of 10.47 mas as seen from Earth, [1] this system is located around 310 light years from the Sun. They are receding with a radial velocity of +2.6 km/s. [6]
This is a visual binary system with the components orbiting each other over a period of roughly 700 years, having an eccentricity of 0.4 and a semimajor axis of 2 arc seconds. [7] The pair have a combined spectral type that matches an A-type main sequence star with a stellar classification of A5 V. [4] The individual components are of estimated types A1 and A6. [5] The primary member, component A, is a magnitude 6.04 [3] star with 1.85 [8] times the mass of the Sun. It is radiating 38 [9] times the Sun's luminosity from its photosphere at an effective temperature of about 7,990 K. [8] The companion, component B, is visual magnitude 7.12. [3]
There are two visual companions: component C is a magnitude 14.3 star at an angular separation of 18.6 arc seconds along a position angle of 266°, as of 2000; component D is magnitude 14.0 with a separation of 29.8 arc seconds along a position angle of 219°, also as of 2000. [11]
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