Groombridge 1618

Groombridge 1618
Groombridge 1618
Location of Groombridge 1618 in the constellation Ursa Major

Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Ursa Major
Right ascension 10h 11m 22.13995s
Declination +49° 27 15.2510
Apparent magnitude (V) +6.60
Characteristics
Spectral type K7.5 Ve
U−B color index +1.27
B−V color index +1.34
Variable type BY Dra, Flare star
Astrometry
Radial velocity (Rv)−26.48±0.12 km/s
Proper motion (μ) RA: −1363.287±0.016 mas/yr
Dec.: −505.770±0.020 mas/yr
Parallax (π)205.3148±0.0224 mas
Distance15.886 ± 0.002 ly
(4.8706 ± 0.0005 pc)
Absolute magnitude (MV)8.11
Details
Mass0.670±0.033 M
Radius0.605±0.02 R
Luminosity (bolometric)0.15 L
Luminosity (visual, LV)0.049 L
Habitable zone inner limit0.398 au
Habitable zone outer limit0.755 au
Surface gravity (log g)4.51; 4.70 cgs
Temperature3,970 K
Metallicity [Fe/H]–0.03 dex
Rotational velocity (v sin i)2.8 km/s
Age6.6 Gyr
Other designations
BD+50° 1725, GJ 380, HD 88230, HIP 49908, SAO 43223, LFT 696, IRAS 10082+4942
Database references
SIMBADdata

Groombridge 1618 is a star in the northern constellation Ursa Major. With an apparent visual magnitude of +6.6, it lies at or below the threshold of stars visible to the naked eye for an average observer. It is relatively close to Earth, at 15.89 light-years (4.87 pc). This is a main sequence star of spectral type K7.5 Ve, having just 67% of the Sun's mass.