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Nearby stars catalogue

G 134-63

Star G 134-63

Red dwarf G 134-63 is located 91 light years away from the Sun. It is suspected double or multiple star of spectral class M5V, that has typically about 25 % of solar mass. For now, there are no known exoplanets in this star system.

Sun distance
91 light years

G 134-63

Red dwarf

Spectral class: M5V

Location +

Right ascension: 2h 59m 46.337s

Declination: 38° 55' 36.3'' (northern hemisphere)

Parallax: 35.9

Sun distance: 90.851 ly | 27.9 pc

Basic characteristic

Mass: 20 % 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 G 134-63

Nearby star G 134-63 is a main sequence star that fuses hydrogen atoms into helium.

       G 134-63 can be found in northern celestial hemisphere.

External sources

Simbad database (G 134-63)

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

BD+39 710	-	3.2 ly
Beta Persei Aa1	3.2 M☉	4.2 ly
UPM J0316+3857	-	5.4 ly
Gaia DR3 235742233662354944	-	6.2 ly
G 78-18	-	7.3 ly

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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.