Star CD-28 302
Red dwarf CD-28 302 is located 38 light years away from the Sun.
It is suspected double or multiple star of spectral class M3V, that has typically about 25 % of solar mass.
For now, there are no known exoplanets in this star system.
More about CD-28 302
Nearby star CD-28 302 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 3402 K (3129 °C), which is about 59 % of Sun's temperature.
CD-28 302 can be found in southern celestial hemisphere, however it is too dim to be seen with the naked eye or even a small telescope.
Other designations of this star
Gaia EDR3 5032683355641241472
External sources
Simbad database (CD-28 302)
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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exoplanets
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Right ascension: 0h 58m 29.507s
Declination: -27° 51' 30.186'' (southern hemisphere)
Parallax: 84.979
Sun distance: 38.381 ly | 11.8 pc
Temperature: 3402 K | 0.59 T Sun
Apparent magnitude (V): 11.8
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