Star MCC 188
Red dwarf MCC 188 is located 36 light years away from the Sun.
It is suspected double or multiple star of spectral class M3Ve, that has typically about 25 % of solar mass.
For now, there are no known exoplanets in this star system.
More about MCC 188
Nearby star MCC 188 is a main sequence star that fuses hydrogen atoms into helium. It is approximately 40 % of the size of Sun and temperature on its surface is around 3431 K (3158 °C), which is about 59 % of Sun's temperature.
MCC 188 can be found in northern celestial hemisphere, you cannot see it with naked eye, but you can observe this star with basic telescope. The star is easily observable from Northern America, Europe and Asia.
Other designations of this star
GJ 735, Gliese 735, AC +08 142-393, 2E 4160, GCRV 68818, HIC 92871, HIP 92871, IRAS 18530+0820, JP11 5167, 2MASS J18552740+0824090, TIC 102107794, TYC 1039-1079-1, V* V1285 Aql, VVO 105, Gaia EDR3 4310275491469537152
External sources
Simbad database (MCC 188)
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: 18h 55m 27.513s
Declination: 8° 24' 7.926'' (equatorial region)
Parallax: 89.906
Sun distance: 36.277 ly | 11.1 pc
Temperature: 3431 K | 0.59 T Sun
Apparent magnitude (V): 10.2
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