KT Lupi is a visual binary star[5] system in the constellation Lupus. It is visible to the naked eye with a combined apparent visual magnitude of 4.55.[3] As of 1983, the pair had an angular separation of 2.19″±0.03″.[10] Based upon an annual parallax shift of 7.6 mas[2] as seen from Earth's orbit, it is located 430 light-years from the Sun. The system is moving further from the Earth with a heliocentric radial velocity of +6.5 km/s.[7] It is a member of the Lower Centaurus–Crux sub-group of the Scorpius–Centaurus association.[5]
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Lupus |
Right ascension | 15h 35m 53.24806s[2] |
Declination | −44° 57′ 30.1982″[2] |
Apparent magnitude (V) | 4.55[3] (4.66 + 6.62)[4] |
Characteristics | |
Spectral type | B3 V + B6 V[5] |
B−V color index | −0.175±0.003[3] |
Variable type | Be[6] |
Astrometry | |
Radial velocity (Rv) | +6.5±2.8[7] km/s |
Proper motion (μ) | RA: −20.53[2] mas/yr Dec.: −21.23[2] mas/yr |
Parallax (π) | 7.62 ± 0.43 mas[2] |
Distance | 430 ± 20 ly (131 ± 7 pc) |
Absolute magnitude (MV) | −1.03[3] |
Details | |
KT Lup A | |
Mass | 5.9±0.1[8] M☉ |
Radius | 3.00±0.06[9] R☉ |
Luminosity | 794+791 −396[10] L☉ |
Surface gravity (log g) | 3.50±0.04[9] cgs |
Temperature | 18,400±184[9] K |
Rotational velocity (v sin i) | 30±0.6[9] km/s |
Age | 21.0±10.6[8] Myr |
KT Lup B | |
Mass | 2.79[11] M☉ |
Other designations | |
Database references | |
SIMBAD | data |
The primary, component A, is a variable Be star,[6] with the variation being modulated by rotation.[13] It is visual magnitude 4.66[4] with a stellar classification of B3 V,[5] matching a B-type main-sequence star. Hiltner et al. (1969) gave a class of B3 IVp,[14] which is still used in some studies.[8][9][10] It is a helium-weak chemically peculiar star showing an enhanced silicon patch near the equator and a silicon-weak region close to the pole.[10] The star is about 21 million years old with nearly six[8] times the mass of the Sun and three times the Sun's radius.[9] It is radiating roughly 794[10] times the Sun's luminosity from its photosphere at an effective temperature of 18,400 K.[9]
The secondary companion, component B, is of magnitude 6.62[4] with a class of B6 V.[5] It has 2.79 times the Sun's mass.[11]