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[1] |
Declination | +49° 27′ 15.2510″[1] |
Apparent magnitude (V) | +6.60[2] |
Characteristics | |
Spectral type | K7.5 Ve[3] |
U−B color index | +1.27[2] |
B−V color index | +1.34[2] |
Variable type | BY Dra,[4] Flare star[5] |
Astrometry | |
Radial velocity (Rv) | −26.48±0.12[1] km/s |
Proper motion (μ) | RA: −1363.287±0.016 mas/yr[1] Dec.: −505.770±0.020 mas/yr[1] |
Parallax (π) | 205.3148 ± 0.0224 mas[1] |
Distance | 15.886 ± 0.002 ly (4.8706 ± 0.0005 pc) |
Absolute magnitude (MV) | 8.11[6] |
Details | |
Mass | 0.670±0.033[7] M☉ |
Radius | 0.605±0.02[7] R☉ |
Luminosity (bolometric) | 0.15[8] L☉ |
Luminosity (visual, LV) | 0.049 L☉ |
Habitable zone inner limit | 0.398[9][note 1] au |
Habitable zone outer limit | 0.755[9] au |
Surface gravity (log g) | 4.51;[10] 4.70[7] cgs |
Temperature | 3,970[10] K |
Metallicity [Fe/H] | –0.03[10] dex |
Rotational velocity (v sin i) | 2.8[11] km/s |
Age | 6.6[8] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
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.
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