Star DG Canis Ven B
Red dwarf DG Canis Ven B is located 60 light years away from the Sun.
It is a single flare star of spectral class M, that has 7 % of solar mass.
For now, there are no known exoplanets in this star system.
Frequently Asked Questions
How far is the DG Canis Ven B system from the Sun?
The DG Canis Ven B system is 60 light years or 18.3 parsecs from the Sun.
What galaxy is the DG Canis Ven B star in?
The DG Canis Ven B is in the Milky Way galaxy just like the Sun.
How many stars are in the DG Canis Ven B system?
The DG Canis Ven B is a single star, there are no other known stars in the system.
What type of star is the DG Canis Ven B?
The star DG Canis Ven B is a Red dwarf star.
What temperature is the DG Canis Ven B?
The primary in the DG Canis Ven 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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Objects listed in the Stellar Catalog often have values that are estimates. These estimates are determined using their known characteristics, such as spectral type, brightness across different wavelengths, distance from a star, and other factors.
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