20 Leonis Minoris
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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 Template: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 Template:Orbitbox end
References
External links
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- Pages with script errors
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- 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
- Pages with reference errors