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Nearby stars catalogue

G 122-8

Star G 122-8

Red dwarf G 122-8 is located 75 light years away from the Sun. It is a single star of spectral class M3.5Ve, that has typically about 25 % of solar mass. For now, there are no known exoplanets in this star system.

Sun distance
75 light years

G 122-8

Red dwarf, High proper motion star

Spectral class: M3.5Ve

Location +

Right ascension: 11h 15m 26.721s

Declination: 41° 5' 12.542'' (northern hemisphere)

Parallax: 43.23

Sun distance: 75.447 ly | 23.1 pc

Basic characteristic

Mass: 30 % M Sun

(estimate)

Size: 30 % 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 122-8

       G 122-8 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 EDR3 765531741023636992

External sources

Simbad database (G 122-8)

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

Gaia database (Gaia EDR3 765531741023636992)

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

MCC 39	-	3 ly
HD 96612	-	4.1 ly
BT Ursae Majoris	-	6.6 ly
LP 263-64	-	6.7 ly
BD+40 2442	-	6.9 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.