Star G 127-22

Red dwarf G 127-22 is located 92 light years away from the Sun. It is a single star of spectral class M3.79, that has typically about 25 % of solar mass. For now, there are no known exoplanets in this star system.

G 127-22

Red dwarf, High proper motion star

Spectral class: M3.79

Location

Right ascension: 22h 22m 51.352s

Declination: 28° 1' 46.372'' (northern hemisphere)

Parallax: 35.314

Sun distance: 92.359 ly | 28.3 pc

Basic characteristic

Mass: 40 % M Sun (estimate)

Size: 100 % R Sun (estimate)

Photometry

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

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

More about G 127-22

       G 127-22 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 1881898955069713024

External sources

Simbad database (G 127-22)

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

Gaia database (Gaia DR3 1881898955069713024)

Archive from the Gaia mission

Class of stars Red dwarf

Red dwarfs are small reddish stars, that are by far the most common type of star in solar neighborhood. Their mass is usually between 10 and 50 % of solar mass.

Closest stars

G 189-11	-	2.5 ly
G 188-40	-	6.9 ly
G 188-39	-	7.7 ly
2MASS J22010456+2413016	-	10 ly
2MASS J21533977+2950053	-	10.8 ly

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