Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Hydra[note 1] |
Right ascension | 08h 53m 36.16047s[1] |
Declination | −03° 29′ 32.1975″[1] |
Apparent magnitude (V) | +18.959[2] |
Characteristics | |
Evolutionary stage | Ultracool dwarf[3][4] |
Spectral type | M9V[3] |
Variable type | Flare star[4] |
Astrometry | |
Radial velocity (Rv) | 7±2[2] km/s |
Proper motion (μ) | RA: −516.605 mas/yr[1] Dec.: −199.652 mas/yr[1] |
Parallax (π) | 115.4876 ± 0.0726 mas[1] |
Distance | 28.24 ± 0.02 ly (8.659 ± 0.005 pc) |
Details | |
Mass | 0.082±0.002[5] M☉ |
Radius | 0.113±0.006[5] R☉ |
Luminosity | 3.39+0.16 −0.15×10−4[6] L☉ |
Surface gravity (log g) | ~5.5[6] cgs |
Temperature | 2,317+61 −56[5] K |
Age | >0.5[4] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
LHS 2065 is a red dwarf star, one of the smallest stars ever found with around 8.2% the mass of the Sun and a diameter only 10% greater than Jupiter.[5] It is one of the few ultracool dwarfs known to have flare activity, emmiting one flare every 33 hours,[4] and is also an active X-ray emitter.[3]
Parallax measurements by the Gaia spacecraft give a distance of 8.66 parsecs (28.2 ly) to LHS 2065.[1] This star was first recorded by the Luyten Half-Second catalogue, a catalogue of stars with proper motions exceding 0.5". The star's main identifier is named after this catalogue.[7] It is located in the Hydra constellation.[a]
This star has a spectral type of M9V,[3] indicating a very cool star at the end of the main sequence. It is among the nearest ultracool dwarfs to Earth.[4] LHS 2065 has an effective temperature of around 2,317 K,[5] 2.5 times less than the Sun. The lack of lithium in the star's atmosphere indicate that it must be over 500 million years old.[4]
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