Ross 128

Ross 128
 Ross 128
Location of Ross 128 in the constellation Virgo

Observation data
Epoch J2000      Equinox J2000
Constellation Virgo
Right ascension 11h 47m 44.39727s
Declination +00° 48 16.4003
Apparent magnitude (V) 11.13
Characteristics
Evolutionary stage Main sequence
Spectral type M4V
U−B color index +2.685
B−V color index +1.59
Variable type Flare star
Astrometry
Radial velocity (Rv)−31.0 km/s
Proper motion (μ) RA: 607.299(34) mas/yr
Dec.: −1223.028(23) mas/yr
Parallax (π)296.3053±0.0302 mas
Distance11.007 ± 0.001 ly
(3.3749 ± 0.0003 pc)
Absolute magnitude (MV)13.53
Details
Mass0.176±0.004 M
Radius0.198±0.007 R
Luminosity (bolometric)0.00366 ± 0.00005 L
Surface gravity (log g)3.40 cgs
Temperature3,189+55
−53
 K
Metallicity [Fe/H]−0.02±0.08 dex
Rotation101–223 days
Rotational velocity (v sin i)2.1±1.0 km/s
Age5.0 Gyr
Other designations
FI Vir, GJ 447, HIP 57548, G 10-50, LFT 852, LHS 315, LSPM J1147+0048, LTT 13240, PLX 2730, Ross 128, Vyssotsky 286
Database references
SIMBADdata
Exoplanet Archivedata

Ross 128 is a red dwarf star in the equatorial zodiac constellation of Virgo, near β Virginis. The apparent magnitude of Ross 128 is 11.13, which is too faint to be seen with the unaided eye. Based upon parallax measurements, the distance of this star from Earth is 11.007 light-years (3.375 parsecs), making it the twelfth closest stellar system to the Solar System. It was first cataloged in 1926 by American astronomer Frank Elmore Ross.