Star V374 Pegasi
Red dwarf V374 Pegasi is located 30 light years away from the Sun.
It is a single flare star of spectral class M3.5 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 V374 Pegasi system from the Sun?
The V374 Pegasi system is 30 light years or 9.1 parsecs from the Sun.
What galaxy is the V374 Pegasi star in?
The V374 Pegasi is in the Milky Way galaxy just like the Sun.
How many stars are in the V374 Pegasi system?
The V374 Pegasi is a single star, there are no other known stars in the system.
What type of star is the V374 Pegasi?
The star V374 Pegasi is a Red dwarf star.
What temperature is star V374 Pegasi?
The star V374 Pegasi has an effective temperature of 3267 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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