GJ 3323

GJ 3323

GJ 3323
Location of GJ 3323 in the constellation Eridanus

Observation data
Epoch J2000      Equinox J2000
Constellation Eridanus
Right ascension 05h 01m 57.42613s
Declination −06° 56 46.3763
Apparent magnitude (V) 12.20
Characteristics
Spectral type M4.0Ve
B−V color index +1.72
Astrometry
Radial velocity (Rv)42.309±0.0809 km/s
Proper motion (μ) RA: −551.746 mas/yr
Dec.: −533.648 mas/yr
Parallax (π)186.0466±0.0277 mas
Distance17.531 ± 0.003 ly
(5.3750 ± 0.0008 pc)
Absolute magnitude (MV)13.57
Details
Mass0.1705±0.0044 M
Radius0.1862±0.0059 R
Luminosity0.003654±0.000052 L
Surface gravity (log g)5.07±0.07 cgs
Temperature3,288±51 K
Metallicity [Fe/H]+0.01±0.16 dex
Rotation88.50 d
Rotational velocity (v sin i)1.0±0.8 km/s
Other designations
GJ 3323, LHS 1723, NLTT 14393, 2MASS J05015746-0656459
Database references
SIMBADdata
Exoplanet Archivedata

GJ 3323, also known as LHS 1723, is a nearby star. It is located in the equatorial constellation Eridanus, about 0.4° to the northwest of the naked eye star Psi Eridani. It is invisible to the naked eye with an apparent visual magnitude 12.20. Parallax measurements give a distance of 17.5 light-years (5.4 parsecs). It is drifting further away with a radial velocity of +42.3 km/s. Roughly 104,000 years ago, the star is believed to have come to within 7.34 ± 0.16 light-years of the Solar System.

The stellar classification of GJ 3323 is M4.0Ve, indicating that it is a red dwarf, with emission lines appearing in its spectrum. It is fully convective and a source of X-ray emission. 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.