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Nearby stars catalogue

PM J10597+5124

Star PM J10597+5124

Red dwarf PM J10597+5124 is located 85 light years away from the Sun. It is a single star, that has typically about 25 % of solar mass. For now, there are no known exoplanets in this star system.

Sun distance
85 light years

PM J10597+5124

Red dwarf, High proper motion star

Location +

Right ascension: 10h 59m 47.045s

Declination: 51° 24' 10.937'' (northern hemisphere)

Parallax: 38.55

Sun distance: 84.606 ly | 25.9 pc

Basic characteristic

Mass: 30 % M Sun

(estimate)

Size: 30 % R Sun

(estimate)

Photometry

Apparent magnitude (V): 13.7

Absolute magnitude (V): 11.7

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 J10597+5124

       PM J10597+5124 can be found in northern celestial hemisphere, however it is too dim to be seen with the naked eye or even a small telescope.

External sources

Simbad database (PM J10597+5124)

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

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

2MASS J11000965+4957470	-	2.6 ly
LP 128-32	-	2.6 ly
UCAC4 709-050017	-	3.3 ly
LZ Ursae Majoris	-	3.4 ly
PM J11072+4851	-	5.6 ly

3D map of stellar neighborhood
List of all nearby stars

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.