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Nearby stars catalogue

GAT 1384

Star GAT 1384

Red dwarf GAT 1384 is located 61 light years away from the Sun. It is a single star of spectral class M6.0V, that has typically about 25 % of solar mass. For now, there are no known exoplanets in this star system.

Sun distance
61 light years

GAT 1384

Red dwarf, High proper motion star

Spectral class: M6.0V

Location +

Right ascension: 21h 58m 36.42s

Declination: 61° 17' 7.768'' (northern hemisphere)

Parallax: 53.662

Sun distance: 60.78 ly | 18.6 pc

Basic characteristic

Mass: 10 % M Sun

(estimate)

Size: 20 % R Sun

(estimate)

Photometry

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 GAT 1384

Nearby star GAT 1384 is a main sequence star that fuses hydrogen atoms into helium.

       GAT 1384 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 2204001126955518592

External sources

Simbad database (GAT 1384)

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

Gaia database (Gaia DR3 2204001126955518592)

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

G 264-22	-	6 ly
Ross 226	-	7.5 ly
LSPM J2127+5553	-	8 ly
Gaia DR2 2206265777300448768	-	8.2 ly
LSPM J2138+5257	-	9.3 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.