Gliese 208

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Gliese 208
V2689OriLightCurve.png
A visual band light curve for V2689 Orionis, adapted from Kiraga (2012) [1]
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
Gliese  208, Gj 208, V2689  Orionis, BD+11°878, HIP  26335, HD  245409, TYC  709-63-1, SAO  94695
Database references
SIMBAD data

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)

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]

Related Research Articles

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<span class="mw-page-title-main">Gliese 105</span> Triple star system in the constellation Cetus

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<span class="mw-page-title-main">GJ 1245</span> Triple star system in the constellation Cygnus

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<span class="mw-page-title-main">Gliese 445</span> Star in the constellation Camelopardalis

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<span class="mw-page-title-main">QZ Puppis</span> Star in the constellation Puppis

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<span class="mw-page-title-main">42 Persei</span> Binary star system in the constellation Perseus

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<span class="mw-page-title-main">21 Persei</span> Star in the constellation Perseus

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<span class="mw-page-title-main">31 Cygni</span> Triple star system in the constellation Cygnus

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<span class="mw-page-title-main">Gliese 908</span> Star in the constellation Pisces

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<span class="mw-page-title-main">Gliese 402</span> Star in the constellation Leo

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<span class="mw-page-title-main">XX Pyxidis</span> Star in the constellation Pyxis

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<span class="mw-page-title-main">DH Tauri</span> Star in the constellation Taurus

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<span class="mw-page-title-main">Gliese 569</span> Nearby red dwarf in the constellation Boötes

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References

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  3. 1 2 3 4 Samus, N. N.; Durlevich, O. V.; et al. (2009). "VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)". VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S. 1. Bibcode:2009yCat....102025S.
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  8. Stephenson, C. B. (1986). "Dwarf K and M stars of high proper motion found in a hemispheric survey". Astronomical Journal. 92: 139. Bibcode:1986AJ.....92..139S. doi: 10.1086/114146 .
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