Star Gliese 358
Red dwarf Gliese 358 is located 31 light years away from the Sun.
It is suspected double or multiple star of spectral class M3 V, that has typically about 25 % of solar mass.
For now, there are no known exoplanets in this star system.
Frequently Asked Questions
How far is the Gliese 358 system from the Sun?
The Gliese 358 system is 31 light years or 9.6 parsecs from the Sun.
What galaxy is the Gliese 358 star in?
The Gliese 358 is in the Milky Way galaxy just like the Sun.
How many stars are in the Gliese 358 system?
The Gliese 358 is a single star, there are no other known stars in the system.
What type of star is the Gliese 358?
The star Gliese 358 is a Red dwarf star.
What temperature is star Gliese 358?
The star Gliese 358 has an effective temperature of 3515 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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