Star TOI 1759
Red dwarf TOI 1759 is located 131 light years away from the Sun.
It is a single star of spectral class M0V, that has 57 % of solar mass.
There is at least one exoplanet in this system.
More about TOI 1759
Star TOI 1759 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 3930 K (3657 °C), which is about 68 % of Sun's temperature.
TOI 1759 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
LSPM J2147+6245, TYC 4266-736-1, TIC 408636441
External sources
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: 21h 47m 24.386s
Declination: 62° 45' 13.733'' (northern hemisphere)
Parallax: 24.922
Sun distance: 130.871 ly | 40.1 pc
Temperature: 3930 K | 0.68 T Sun
Luminosity: 0.089 L Sun
Apparent magnitude (V): 11.9
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