20 Leonis Minoris
Star in the constellation Leo Minor / From Wikipedia, the free encyclopedia
20 Leonis Minoris is a binary star system in the northern constellation of Leo Minor. It is faintly visible to the naked eye, having an apparent visual magnitude of +5.4.[2] Based upon an annual parallax shift of 66.46 mas, it is located 49 light years from the Sun. The star has a relatively high proper motion[3] and is moving away from the Sun with a radial velocity of +56 km/s.[6] The system made its closest approach about 150,000 years ago when it came within 32.2 ly (9.86 pc).[13]
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Leo Minor |
Right ascension | 10h 01m 00.65765s[1] |
Declination | +31° 55′ 25.2151″[1] |
Apparent magnitude (V) | +5.40[2] |
Characteristics | |
Spectral type | G3 Va Hδ1[3] + M7 V[4] |
U−B color index | +0.27[5] |
B−V color index | +0.65[5] |
Astrometry | |
Radial velocity (Rv) | +55.96±0.09[6] km/s |
Proper motion (μ) | RA: −527.63±0.30[1] mas/yr Dec.: −429.42±0.18[1] mas/yr |
Parallax (π) | 66.46 ± 0.32 mas[1] |
Distance | 49.1 ± 0.2 ly (15.05 ± 0.07 pc) |
Absolute magnitude (MV) | 4.46[7] |
Details | |
20 LMi A | |
Mass | 1.12[8] M☉ |
Radius | 1.247±0.021[9] R☉ |
Luminosity | 1.378±0.027[9] L☉ |
Temperature | 5,735±5.6[10] K |
Rotation | 10.64±0.14 d[2] |
Age | 6.2–7.7[11] Gyr |
20 LMi B | |
Mass | 0.11[8] M☉ |
Rotation | 19.2687 d[4] |
Other designations | |
Database references | |
SIMBAD | data |
The primary member of this system is a G-type main-sequence star with a stellar classification of G3 Va Hδ1.[3] It has 12% more mass and a 25% larger radius than the Sun. The star is about seven[11] billion years old and is spinning with a rotation period of 10.6 days.[2] The small companion is an active red dwarf star that has a relatively high metallicity.[14] The two stars are currently separated by 14.5 arc seconds, corresponding to a projected separation of 2016 AU.[8]
In 2020, a candidate exoplanet was detected orbiting 20 Leonis Minoris (HD 86728). With a minimum mass of 0.032 MJ (10.2 ME) and an orbital period of 31 days, this would most likely be a hot Neptune.[15]
Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b (unconfirmed) | ≥0.032+0.005 −0.005 MJ |
0.2003+0.00007 −0.00007 |
31.15+0.02 −0.02 |
0.2+0.2 −0.1 |
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