Star TOI 3235
Red dwarf TOI 3235 is located 237 light years away from the Sun.
It is a single star of spectral class M4V, that has 39 % of solar mass.
There is at least one exoplanet in this system.
Frequently Asked Questions
How far is the TOI 3235 system from the Sun?
The TOI 3235 system is 237 light years or 72.6 parsecs from the Sun.
What galaxy is the TOI 3235 star in?
The TOI 3235 is in the Milky Way galaxy just like the Sun.
How many stars are in the TOI 3235 system?
The TOI 3235 is a single star, there are no other known stars in the system.
What type of star is the TOI 3235?
The star TOI 3235 is a Red dwarf star.
What temperature is star TOI 3235?
The star TOI 3235 has an effective temperature of 3388 K. Find out more about the temperature of stars in
Stellar guide
Class of stars Red dwarf
Red dwarfs are small, cool stars with surface temperatures of about 2,000–3,800 K, much cooler than the Sun. They usually have 8–50% of the Sun’s mass and shine very faintly, sometimes at just a tiny fraction of the Sun’s brightness. Classified mainly as spectral type M, they are the most common stars in the Milky Way, making up roughly 70–75% of its stellar population.
They fuse hydrogen slowly through the proton–proton chain and are fully convective, which allows them to use their fuel very efficiently. As a result, red dwarfs can live for tens of billions to trillions of years—far longer than the Sun. Many exoplanets orbit red dwarfs, including some in close habitable zones, though strong stellar activity can affect planetary environments.
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