Ross 154

Ross 154
Ross 154
Location of Ross 154 in the constellation Sagittarius

Observation data
Epoch J2000      Equinox J2000
Constellation Sagittarius
Right ascension 18h 49m 49.36378s
Declination −23° 50′ 10.4474″
Apparent magnitude (V) 10.44
Characteristics
Spectral type M3.5V
B−V color index 1.76
Variable type Flare star
Astrometry
Radial velocity (Rv)−11.12±0.57 km/s
Proper motion (μ) RA: +639.368 mas/yr
Dec.: −193.958 mas/yr
Parallax (π)336.0266±0.0317 mas
Distance9.7063 ± 0.0009 ly
(2.9760 ± 0.0003 pc)
Absolute magnitude (MV)13.07
Details
Mass0.177±0.004 M
Radius0.200±0.008 R
Luminosity0.004015±0.000048 L
Surface gravity (log g)5.00±0.05 cgs
Temperature3,248+68
−66
 K
Metallicity [Fe/H]−0.25 dex
Rotation2.848±0.001 days
Rotational velocity (v sin i)3.5±1.5 km/s
Ageunder 1 Gyr
Other designations
CD−23°14742, GCTP 4338, GJ 729, HIP 92403, LHS 3414, V1216 Sagittarii
Database references
SIMBADdata

Ross 154 (V1216 Sgr) is a red dwarf star in the southern zodiac constellation of Sagittarius. It has an apparent visual magnitude of 10.44, making it much too faint to be seen with the naked eye. At a minimum, viewing Ross 154 requires a telescope with an aperture of 6.5 cm (3 in) under ideal conditions. The distance to this star can be estimated from parallax measurements, which places it at 9.71 light-years (2.98 parsecs) away from Earth. It is the nearest star in the southern constellation Sagittarius, and one of the nearest stars to the Sun.