Star Gliese 3192 B
Red dwarf Gliese 3192 B is located 23 light years away from the Sun.
It is suspected double or multiple star of spectral class M3V, that has 25 % of solar mass.
For now, there are no known exoplanets in this star system.
Frequently Asked Questions
How far is the Gliese 3192 B system from the Sun?
The Gliese 3192 B system is 23 light years or 7.2 parsecs from the Sun.
What galaxy is the Gliese 3192 B star in?
The Gliese 3192 B is in the Milky Way galaxy just like the Sun.
How many stars are in the Gliese 3192 B system?
The Gliese 3192 B is a single star, there are no other known stars in the system.
What type of star is the Gliese 3192 B?
The star Gliese 3192 B is a Red dwarf star.
What temperature is the Gliese 3192 B?
The primary in the Gliese 3192 B system has an effective temperature of K ( °C). 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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