Star LHS 1478
Red dwarf LHS 1478 is located 59 light years away from the Sun.
It is a single star of spectral class M3.5V, that has 24 % of solar mass.
There is at least one exoplanet in this system.
Frequently Asked Questions
How far is the LHS 1478 system from the Sun?
The LHS 1478 system is 59 light years or 18.2 parsecs from the Sun.
What galaxy is the LHS 1478 star in?
The LHS 1478 is in the Milky Way galaxy just like the Sun.
How many stars are in the LHS 1478 system?
The LHS 1478 is a single star, there are no other known stars in the system.
What type of star is the LHS 1478?
The star LHS 1478 is a Red dwarf star.
What temperature is star LHS 1478?
The star LHS 1478 has an effective temperature of 3381 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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