GJ 3929

GJ 3929

Artist's impression and size comparison of the two planets in the GJ 3929 system with Earth
Observation data
Epoch J2000      Equinox J2000
Constellation Corona Borealis
Right ascension 15h 58m 18.80s
Declination +35° 24 24.3
Apparent magnitude (V) 12.67
Characteristics
Spectral type M3.5V
Astrometry
Radial velocity (Rv)10.14 km/s
Proper motion (μ) RA: −143.059 mas/yr
Dec.: +318.120 mas/yr
Parallax (π)63.1727±0.038 mas
Distance51.63 ± 0.03 ly
(15.830 ± 0.010 pc)
Absolute magnitude (MV)11.7
Details
Mass0.313+0.027
−0.022
 M
Radius0.32±0.01 R
Luminosity0.0109+0.0005
−0.0004
 L
Surface gravity (log g)4.89±0.05 cgs
Temperature3,384±88 K
Metallicity [Fe/H]−0.02±0.12 dex
Rotation122±13 d
Rotational velocity (v sin i)<2 km/s
Age2.2 – 11.2 Gyr
Other designations
TOI-2013, TIC 188589164, 2MASS J15581883+3524236, Gaia DR3 1372215976327300480, G 180-18
Database references
SIMBADdata

GJ 3929, also known as Gliese 3929 and TOI-2013, is a red dwarf star located 51.6 light-years from Earth, in the constellation Corona Borealis. With an apparent magnitude of 12, it is not visible to the naked eye. In 2022, two exoplanets were detected orbiting the star.