Star Gliese 190
Red dwarf Gliese 190 is located 30 light years away from the Sun.
It is suspected double or multiple star of spectral class M3.5 V, that has typically about 25 % of solar mass.
For now, there are no known exoplanets in this star system.
More about Gliese 190
Nearby star Gliese 190 is a main sequence star that fuses hydrogen atoms into helium. It is approximately 30 % of the size of Sun and temperature on its surface is around 3109 K (2836 °C), which is about 54 % of Sun's temperature.
Gliese 190 can be found in southern celestial hemisphere, you cannot see it with naked eye, but you can observe this star with basic telescope. The star is also observable from Northern America, Europe and Asia.
Other designations of this star
L 737-9, LHS 203, HIC 23932, HIP 23932, LFT 391, LP 777-36, LTT 2179, NLTT 14559, 2MASS J05083500-1810178, Gaia EDR3 2976507997939000064
External sources
Simbad database (L 737-9)
Astronomical database SIMBAD (the Set of Identifications, Measurements and Bibliography for Astronomical Data)
Class of stars Red dwarf
Red dwarfs are small reddish stars, that are by far the most common type of star in solar neighborhood. Their mass is usually between 10 and 50 % of solar mass.
stars
exoplanets
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Right ascension: 5h 8m 35.616s
Declination: -18° 10' 41.783'' (equatorial region)
Parallax: 108.325
Sun distance: 30.109 ly | 9.2 pc
Temperature: 3109 K | 0.54 T Sun
Apparent magnitude (V): 10.3
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