Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Scorpius |
Right ascension | 16h 08m 43.7s[1] |
Declination | −23° 41′ 07.5″[1] |
Apparent magnitude (V) | +5.88[1] (5.87 to 5.90)[2] |
Characteristics | |
Spectral type | B9V[1] B9 Mn P Ga[3] B9 IVn + Ap(Si)s[4] |
U−B color index | +0.02[1] |
B−V color index | −0.31[1] |
Variable type | α2 CVn[2] |
Astrometry | |
Radial velocity (Rv) | −16.0[1] km/s |
Proper motion (μ) | RA: −10.09±0.22[5] mas/yr Dec.: −26.09±0.18[5] mas/yr |
Parallax (π) | 6.4762 ± 0.1839 mas[5] |
Distance | 500 ± 10 ly (154 ± 4 pc) |
Absolute magnitude (MV) | −0.33±0.07[6] |
Details | |
Mass | 3.46±0.14 M☉[7] 2.5[6] M☉ |
Radius | 3.2[8] R☉ |
Luminosity | 190 ± 40[7] L☉ |
Surface gravity (log g) | 3.76[8] cgs |
Temperature | 12,430±460[7] K |
Metallicity [Fe/H] | +0.033[9] dex |
Rotational velocity (v sin i) | 45.0±1.5[7] km/s |
Age | 10±3[6] Myr |
Other designations | |
Database references | |
SIMBAD | data |
HIP 79098 is a binary star in the constellation Scorpius. It has a visual apparent magnitude of +5.88,[1] being visible to the naked eye under very dark skies. From parallax measurements by the Gaia spacecraft, it is located approximately 500 light-years (154 parsecs) from Earth.[5]
This system consists of a chemically peculiar B-type star, plus a spectroscopic companion of unknown type. Two additional distant red dwarfs may be part of the system, at separations of 9,500 and 12,900 AU. In 2019, a brown dwarf was discovered orbiting the central binary at a distance of about 350 AU.[6]
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