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Red dwarf star in the constellation Orion From Wikipedia, the free encyclopedia
Gliese 208 (Gj 208) is a red dwarf star with an apparent magnitude of 8.9. It is 37 light years away in the constellation of Orion. It is an extremely wide binary with 2MASS J0536+1117, an M4 star 2.6 arcminutes away (at least 0.028 light years)
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Orion |
Right ascension | 05h 36m 30.991s[2] |
Declination | +11° 19′ 40.33″[2] |
Apparent magnitude (V) | 8.80 - 9.05[3] |
Characteristics | |
Spectral type | M0.0 Ve[4] |
Variable type | RS CVn[3] |
Astrometry | |
Radial velocity (Rv) | 21.772[5] km/s |
Proper motion (μ) | RA: −2.811 ± 0.080[2] mas/yr Dec.: −56.368 ± 0.060[2] mas/yr |
Parallax (π) | 87.66 ± 0.29 mas[2] |
Distance | 37.2 ± 0.1 ly (11.41 ± 0.04 pc) |
Absolute magnitude (MV) | 8.6 |
Details | |
Mass | 0.646[6] M☉ |
Radius | 0.601[6] R☉ |
Luminosity | 0.08[7] L☉ |
Temperature | 3,966[6] K |
Metallicity [Fe/H] | +0.05[6] dex |
Age | 2.7[6] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
The spectral type of Gj 208 has variously been described between K6 and M1.[8][9][10] Two of the most recent observations give a statistically calculated spectral type of K7.9[6] or a more traditional classification of M0.0 Ve.[4] It is a cool dwarf star and probably a spectroscopic binary.[3]
Calculations from 2010 suggest that this star passed as close as 1.537 parsecs (5.0 light-years) from the Sun about 500,000 years ago.[11]
GJ 208 is an RS Canum Venaticorum variable, close binary systems which show small amplitude brightness changes caused by chromospheric activity. Its visual magnitude varies by about a quarter magnitude with a period of 12.285 days.[3]
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