Star LSPM J0804+1116
The TOI-6981 system features a Red dwarf star of spectral type M4. The host star possesses a radius of 0.304 solar radii and a mass of 0.296 solar masses, with a surface temperature of 3215 K. It serves as the host to the sub-Neptune planet TOI-6981 b, which orbits within the cold region of the system corresponding to the water ice line.
Frequently Asked Questions
How far is the LSPM J0804+1116 system from the Sun?
The LSPM J0804+1116 system is 83 light years or 25.3 parsecs from the Sun.
What galaxy is the LSPM J0804+1116 star in?
The LSPM J0804+1116 is in the Milky Way galaxy just like the Sun.
How many stars are in the LSPM J0804+1116 system?
The LSPM J0804+1116 is a single star, there are no other known stars in the system.
What type of star is the LSPM J0804+1116?
The star LSPM J0804+1116 is a Red dwarf star.
What temperature is star LSPM J0804+1116?
The star LSPM J0804+1116 has an effective temperature of 3215 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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