Location of GJ 3323 in the constellation Eridanus | |
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Eridanus |
Right ascension | 05h 01m 57.42613s[1] |
Declination | −06° 56′ 46.3763″[1] |
Apparent magnitude (V) | 12.20[2] |
Characteristics | |
Spectral type | M4.0Ve[3] |
B−V color index | +1.72[2] |
Astrometry | |
Radial velocity (Rv) | 42.309±0.0809[2] km/s |
Proper motion (μ) | RA: −551.746 mas/yr[1] Dec.: −533.648 mas/yr[1] |
Parallax (π) | 186.0466 ± 0.0277 mas[1] |
Distance | 17.531 ± 0.003 ly (5.3750 ± 0.0008 pc) |
Absolute magnitude (MV) | 13.57[3] |
Details[4] | |
Mass | 0.1705±0.0044 M☉ |
Radius | 0.1862±0.0059 R☉ |
Luminosity | 0.003654±0.000052 L☉ |
Surface gravity (log g) | 5.07±0.07 cgs |
Temperature | 3,288±51 K |
Metallicity [Fe/H] | +0.01±0.16 dex |
Rotation | 88.50 d[5] |
Rotational velocity (v sin i) | 1.0±0.8[3] km/s |
Other designations | |
Database references | |
SIMBAD | data |
GJ 3323 (also known as LHS 1723) is a nearby single[7] star located in the equatorial constellation Eridanus, about 0.4° to the northwest of the naked eye star Psi Eridani.[8] It is invisible to the naked eye with an apparent visual magnitude 12.20.[2] Parallax measurements give a distance estimate of 17.5 light-years (5.4 parsecs) from the Sun.[1] It is drifting further away with a radial velocity of +42.3 km/s.[2] Roughly 104,000 years ago, the star is believed to have come to within 7.34 ± 0.16 light-years of the Solar System.[9]
The stellar classification of GJ 3323 is M4.0Ve,[3] indicating that it is a red dwarf, with emission lines appearing in its spectrum.[2] It is fully convective and a source of X-ray emission.[5] The star has 17% of the Sun's mass, 19% of the radius of the Sun, and just 0.4% of the Sun's luminosity.[4]
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