HD 134687 (e Lupi) is a binary star system in the southern constellation Lupus. It is visible to the naked eye with an apparent visual magnitude of 4.81.[2] The distance to HD 134687 can be estimated from its annual parallax shift of 7.6 mas,[1] yielding roughly 430 light years. It is a member of the ~11 million year old Upper Centaurus–Lupus subgroup of the Scorpius–Centaurus association, the closest OB association to the Sun.[11]
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Lupus |
Right ascension | 15h 12m 49.58802s[1] |
Declination | −44° 30′ 01.4867″[1] |
Apparent magnitude (V) | 4.81[2] |
Characteristics | |
Spectral type | B3 IV/V[3] |
B−V color index | −0.177±0.011[4] |
Astrometry | |
Radial velocity (Rv) | +13.5±7.4[5] km/s |
Proper motion (μ) | RA: −22.015[1] mas/yr Dec.: −22.164[1] mas/yr |
Parallax (π) | 7.6373 ± 0.9664 mas[1] |
Distance | approx. 430 ly (approx. 130 pc) |
Absolute magnitude (MV) | −1.11[4] |
Orbit[6] | |
Period (P) | 0.901407 d |
Eccentricity (e) | ≤ 0.03 |
Periastron epoch (T) | 0.366 |
Details | |
e Lup A | |
Mass | 6.0±0.1[7] M☉ |
Radius | 7.1[8] R☉ |
Luminosity (bolometric) | 997[2] L☉ |
Temperature | 17,100[2] K |
Rotational velocity (v sin i) | 13[9] km/s |
Age | 20.3±4.8 Myr |
Other designations | |
Database references | |
SIMBAD | data |
This is a single-lined spectroscopic binary star system. The pair have a nearly circular orbit with an eccentricity of at or below 0.03 and a period of 0.901407 days (21.6338 h). The primary has an a sin i value of 2.735×105 km, which only gives a lower bound for the semimajor axis a since the orbital inclination i to the line of sight is unknown.[6] The system is a source for X-ray emission.[12]
The visible component has a stellar classification of B3 IV/V,[3] matching a B-type star showing a spectrum with mixed traits of a main sequence and a subgiant star. It is 20 million years old with a projected rotational velocity of 13 km/s.[9] The star has 6.0[7] times the mass of the Sun and 7.1[8] times the Sun's radius. It is radiating 997[2] times the Sun's luminosity from its photosphere at an effective temperature of 17,100 K.[2]