LHS 2065
Red dwarf star in the constellation Hydra
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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.[8] It is one of the few ultracool dwarfs known to have flare activity, emitting one flare every 33 hours,[6] and is also an active X-ray emitter.[5]
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Hydra[2] |
| Right ascension | 08h 53m 36.16047s[3] |
| Declination | −03° 29′ 32.1975″[3] |
| Apparent magnitude (V) | +18.959[4] |
| Characteristics | |
| Evolutionary stage | main sequence[5] |
| Spectral type | M9V[5] |
| Variable type | Flare star[6] |
| Astrometry | |
| Radial velocity (Rv) | 7±2[7] km/s |
| Proper motion (μ) | RA: −516.605 mas/yr[3] Dec.: −199.652 mas/yr[3] |
| Parallax (π) | 115.4876±0.0726 mas[3] |
| Distance | 28.24 ± 0.02 ly (8.659 ± 0.005 pc) |
| Details | |
| Mass | 0.082±0.002[8] M☉ |
| Radius | 0.113±0.006[8] R☉ |
| Luminosity | 3.39+0.16 −0.15×10−4[9] L☉ |
| Surface gravity (log g) | ~5.5[9] cgs |
| Temperature | 2,317+61 −56[8] K |
| Age | >0.5[6] Gyr |
| Other designations | |
| GJ 3517, LHS 2065, LP 666-9, TIC 7975441, 2MASS J08533619-0329321[10] | |
| Database references | |
| SIMBAD | data |
Parallax measurements by the Gaia spacecraft give a distance of 8.66 parsecs (28.2 ly) to LHS 2065.[3] This star was first recorded by the Luyten Half-Second catalogue, a catalogue of stars with proper motions exceeding 0.5". The star's main identifier is named after this catalogue.[11] It is located in the Hydra constellation.[2]
This star has a spectral type of M9V,[5] indicating a very cool star at the end of the main sequence. It is among the nearest ultracool dwarfs to Earth.[6] LHS 2065 has an effective temperature of around 2,317 K,[8] 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.[6]