Star LP 890-9
Red dwarf LP 890-9 is located 105 light years away from the Sun.
It is a single star of spectral class M6 D, that has 12 % of solar mass.
There are multiple known exoplanets in this system.
Frequently Asked Questions
How far is the LP 890-9 system from the Sun?
The LP 890-9 system is 105 light years or 32.3 parsecs from the Sun.
What galaxy is the LP 890-9 star in?
The LP 890-9 is in the Milky Way galaxy just like the Sun.
How many stars are in the LP 890-9 system?
The LP 890-9 is a single star, there are no other known stars in the system.
What type of star is the LP 890-9?
The star LP 890-9 is a Red dwarf star.
What temperature is star LP 890-9?
The star LP 890-9 has an effective temperature of 2850.0 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.
Get your next news from nearby stars
Stellar Catalog brings the stars from our galaxy to you. Discover their position, physical properties and whether there are any exoplanets or disks orbiting them. The data in Stellar Catalog come from respectable sources like Gaia space telescope, or SIMBAD database.