Star TOI 620
Red dwarf TOI 620 is located 108 light years away from the Sun.
It is a single star of spectral class M2.5V, that has 58 % of solar mass.
There are multiple known exoplanets in this system.
More about TOI 620
Star TOI 620 is a main sequence star that fuses hydrogen atoms into helium. It is approximately 60 % of the size of Sun and temperature on its surface is around 3708 K (3435 °C), which is about 64 % of Sun's temperature.
TOI 620 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
TIC 296739893, G 161-32, NLTT 21863, Gaia EDR3 5738284016370287616, 2MASS J09284158-1209551
External sources
Simbad database (G 161-32)
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: 9h 28m 41.635s
Declination: -12° 9' 55.75'' (equatorial region)
Parallax: 30.283
Sun distance: 107.703 ly | 33 pc
Temperature: 3708 K | 0.64 T Sun
Age: 7.2 billions years | 1.57 Sun
Luminosity: 0.0515 L Sun
Apparent magnitude (V): 12.3
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