20 Leonis Minoris
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Leo Minor |
| Right ascension | Template:RA[1] |
| Declination | Template:DEC[1] |
| Apparent magnitude (V) | +5.40[2] |
| Characteristics | |
| Spectral type | G3 Va Hδ1[3] + M7 V[4] |
| U−B Template:Engvar | +0.27[5] |
| B−V Template:Engvar | +0.65[5] |
| Astrometry | |
| Radial velocity (Rv) | Script error: No such module "val".[6] km/s |
| Proper motion (μ) | RA: Script error: No such module "val". mas/yr[1] Dec.: Script error: No such module "val". mas/yr[1] |
| Parallax (π) | 66.9958±0.0921 mas[1] |
| Distance | Template:Rnd ± Template:Rnd ly (Template:Rnd ± Template:Rnd pc) |
| Absolute magnitude (MV) | 4.46[7] |
| Details | |
| 20 LMi A | |
| Mass | Script error: No such module "val".[8] Template:Solar mass |
| Radius | Script error: No such module "val".[8] Template:Solar radius |
| Luminosity | Script error: No such module "val".[8] Template:Solar luminosity |
| Surface gravity (log g) | Script error: No such module "val".[8] cgs |
| Temperature | Script error: No such module "val".[9] K |
| Metallicity [Fe/H] | Script error: No such module "val".[8] dex |
| Rotation | Script error: No such module "val".[2] |
| Rotational velocity (v sin i) | Script error: No such module "val".[8] km/s |
| Age | 6.2–7.7[10] Gyr |
| 20 LMi B | |
| Mass | 0.11[11] Template:Solar mass |
| Temperature | Script error: No such module "val".[12] K |
| Metallicity [Fe/H] | Script error: No such module "val".[12] dex |
| Rotation | 19.2687 d[4] |
| Other designations | |
| Template:Odlist[13] | |
| Database references | |
| SIMBAD | data |
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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 66.996 mas, it is located 48.7 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 Script error: No such module "convert"..[14]
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[10] 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.[15] The two stars are currently separated by 14.5 arc seconds, corresponding to a projected separation of 2016 AU.[11]
Planetary system
A candidate exoplanet orbiting 20 Leonis Minoris A (HD 86728) was first detected in 2020,[17] and confirmed in 2024 as the first discovery of the NEID Earth Twin Survey (NETS). With a minimum mass of Template:Earth mass and an orbital period of 31 days, this is most likely a hot Neptune-type planet.[8]
Template:OrbitboxPlanet begin Template:OrbitboxPlanet
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References
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- ↑ a b c d Template:Cite Gaia DR3
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- ↑ Template:Cite simbad
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External links
- Script error: No such module "citation/CS1".
- Pages with script errors
- Pages with broken file links
- G-type main-sequence stars
- M-type main-sequence stars
- Solar analogs
- Binary stars
- Leo Minor
- Durchmusterung objects
- Flamsteed objects
- Gliese and GJ objects
- Henry Draper Catalogue objects
- Hipparcos objects
- Bright Star Catalogue objects
- Planetary systems with one confirmed planet