Star G 107-69
Red dwarf G 107-69 is located 37 light years away from the Sun.
It is a single star of spectral class M4V, that has typically about 25 % of solar mass.
For now, there are no known exoplanets in this star system.
More about G 107-69
Nearby star G 107-69 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 3293 K (3020 °C), which is about 57 % of Sun's temperature.
G 107-69 can be found in northern celestial hemisphere, however it is too dim to be seen with the naked eye or even a small telescope.
Other designations of this star
LHS 229, G 111-7, G 193-50, GJ 275.2 A, Gliese 275.2 A, 2MASS J07304280+4811599, NLTT 17949, TIC 328328639, WISEA J073042.55+481145.2, Gaia EDR3 975968718869126144
External sources
Simbad database (G 107-69)
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
en
Right ascension: 7h 30m 42.463s
Declination: 48° 11' 38.234'' (northern hemisphere)
Parallax: 88.723
Sun distance: 36.761 ly | 11.3 pc
Temperature: 3293 K | 0.57 T Sun
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