Star HD 232979
Red dwarf HD 232979 is located 32 light years away from the Sun.
It is a single star of spectral class M0.5V , that has typically about 25 % of solar mass.
For now, there are no known exoplanets in this star system.
More about HD 232979
Nearby star HD 232979 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 4034 K (3761 °C), which is about 70 % of Sun's temperature.
HD 232979 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
HD 232979, TYC 3732-542-1, HIP 21553, Gaia EDR3 272855565763652480
External sources
Simbad database (HD 232979)
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.
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Right ascension: 4h 37m 41.475s
Declination: 52° 53' 29.411'' (northern hemisphere)
Parallax: 100.916
Sun distance: 32.32 ly | 9.9 pc
Temperature: 4034 K | 0.7 T Sun
Luminosity: 0.08 L Sun
Apparent magnitude (V): 8.6
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