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Nearby stars catalogue

PM J10581+5057

Star PM J10581+5057

Red dwarf PM J10581+5057 is located 90 light years away from the Sun. It is a single star of spectral class M3.52, that has typically about 25 % of solar mass. For now, there are no known exoplanets in this star system.

Sun distance
90 light years

PM J10581+5057

Red dwarf

Spectral class: M3.52

Location +

Right ascension: 10h 58m 7.481s

Declination: 50° 57' 3.496'' (northern hemisphere)

Parallax: 36.137

Sun distance: 90.255 ly | 27.7 pc

Basic characteristic

Mass: 40 % M Sun

(estimate)

Size: 100 % R Sun

(estimate)

Photometry

Apparent magnitude (V): 13.6

Absolute magnitude (V): 11.4

Absolute stellar magnitude in different parts of the electromagnetic spectrum from infrared (K band) to ultraviolet (U band).

K
2.1

H
1.6

J
1.2

Grp
0.8

I
0.8

G
0.6

V
0.5

Gbp
0.5

B
0.4

U
0.3

More about PM J10581+5057

       PM J10581+5057 can be found in northern celestial hemisphere, however it is too dim to be seen with the naked eye or even a small telescope.

Other designations of this star
Gaia DR3 836099398022603776

External sources

Simbad database (PM J10581+5057)

Astronomical database SIMBAD (the Set of Identifications, Measurements and Bibliography for Astronomical Data)

Gaia database (Gaia DR3 836099398022603776)

Archive from the Gaia mission

Class of stars Red dwarf

Red dwarfs are small, relatively cool, reddish stars. They are by far the most common type of star in the solar neighborhood. Their mass typically ranges from about 8% to 50% of the Sun's mass.

Closest stars

UCAC4 709-050017	-	3.5 ly
LZ Ursae Majoris	-	3.8 ly
PM J11072+4851	-	4.4 ly
LP 128-32	-	4.7 ly
BD+49 2004	-	4.7 ly

3D map of stellar neighborhood
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About Stellar Catalog

Working with real data

Data in Stellar Catalog come from trusted scientific sources. Primary source is Gaia space telescope mapping the stars in Milky Way. Other sources include research papers, Simbad catalog and Exoplanet.eu database.

Estimated values

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.

Fresh and validated

Stellar Catalog is continuously updated with new information from research papers. Stellar and planetary data are validated by automatic processes as well as humans.