Star TOI-270
Red dwarf TOI-270 is located 73 light years away from the Sun.
It is a single star of spectral class M3.0V C, that has 40 % of solar mass.
There are multiple known exoplanets in this system.
More about TOI-270
Nearby star TOI-270 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 3551 K (3278 °C), which is about 61 % of Sun's temperature.
TOI-270 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
L 231-32, LEHPM 3808, 2MASS J04333970-5157222, TIC 259377017, UCAC4 191-004642, Gaia EDR3 4781196115469953024
External sources
Simbad database (L 231-32)
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.
stars
exoplanets
en
Right ascension: 4h 33m 39.87s
Declination: -51° 57' 26.752'' (southern hemisphere)
Parallax: 44.49
Sun distance: 73.31 ly | 22.5 pc
Temperature: 3551 K | 0.61 T Sun
Apparent magnitude (V): 12.6
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