Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Leo |
Right ascension | 09h 58m 13.37557s[1] |
Declination | +12° 26′ 41.2865″[1] |
Apparent magnitude (V) | 5.15[2] |
Characteristics | |
Spectral type | B6 IV[3] |
U−B color index | −0.13[2] |
B−V color index | −0.04[2] |
Astrometry | |
Radial velocity (Rv) | +14.4[4] km/s |
Proper motion (μ) | RA: −25.66[1] mas/yr Dec.: −15.56[1] mas/yr |
Parallax (π) | 6.53 ± 0.24 mas[1] |
Distance | 500 ± 20 ly (153 ± 6 pc) |
Absolute magnitude (MV) | −0.66[5] |
Orbit[6] | |
Period (P) | 137.2978 d |
Eccentricity (e) | 0.7 |
Longitude of the node (Ω) | 293.7° |
Periastron epoch (T) | 2419815.9 JD |
Semi-amplitude (K1) (primary) | 20 km/s |
Details | |
Mass | 3.37±0.05[7] M☉ |
Radius | 2.3[8] R☉ |
Luminosity | 244[7] L☉ |
Temperature | 9,552[9] K |
Rotational velocity (v sin i) | 100[7] km/s |
Other designations | |
Database references | |
SIMBAD | data |
ν Leonis, Latinised as Nu Leonis, is a binary star system in the zodiac constellation of Leo. It is faintly visible to the naked eye with an apparent visual magnitude of 5.15;[2] parallax measurements[1] indicate it is around 500 light years away. At this distance, the visual extinction from interstellar dust is 0.33 magnitudes.[11]
It is 0.05 degree north of the ecliptic, so it can be occulted by the moon or planets.
This is a single-lined spectroscopic binary system with an orbital period of 137.3 days and an eccentricity of 0.7.[6] The primary component is a B-type subgiant star with a stellar classification of B6 IV.[3] It has about 3.37 times the mass of the Sun,[7] 2.3 times the Sun's radius,[8] and radiates 244[7] times the luminosity of the Sun from an outer atmosphere with an effective temperature of 9,552 K.[9] The rotation rate is moderate with a projected rotational velocity of 100 km/s.[7] Little is known about the companion.[6]
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