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Star Gliese 422

Red dwarf Gliese 422 is located 41 light years away from the Sun. It is a single star of spectral class M3.5 D, that has 35 % of solar mass. There is at least one exoplanet in this system.
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Sun distance
41 light years

Gliese 422

Red dwarf, High proper motion star
Spectral class: M3.5 D

Location +

Ascension iconRight ascension: 11h 15m 55.307s
Declination iconDeclination: -57° 32' 32.634'' (southern hemisphere)
Parallax iconParallax: 78.892
Distance iconSun distance: 41.342 ly | 12.7 pc
Star position
The position of a star tells us where it appears in the sky, similar to how we use coordinates like latitude and longitude on Earth. In astronomy, the three main coordinates are right ascension, declination and distance. .. icon More about Star position in StellarGuide

Basic characteristic

icon weight
Mass: 35 % M Sun
| 367 M Jupiter
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Star mass
Mass of the star Gliese 422 is 0.35 solar masses.

The mass of a star is the total amount of matter it contains. It is one of the most important properties of a star, as it determines almost everything about how the star lives, changes, and dies. In astronomy, star mass is usually measured in solar masses (M☉) — where 1 solar mass is equal to the mass of our Sun... icon More about Star mass in StellarGuide
temperature icon
Temperature: 3501 K | 0.61 T Sun
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Star temperature
Surface temperature of Gliese 422 is 3501 K, which is 61 % of the temperature on the surface of the Sun.

The temperature of a star refers to the temperature at its surface, also called the photosphere. It is measured in kelvins (K), the standard unit for temperature in astronomy. A star’s temperature tells us a lot about its physical properties and where it stands in its evolutionary stage... icon More about Star temperature in StellarGuide

Photometry

Magnitude iconApparent magnitude (V): 11.5
Magnitude iconAbsolute magnitude (V): 11
Absolute stellar magnitude in different parts of the electromagnetic spectrum from infrared (K band) to ultraviolet (U band).
5
10
15
20
25
30
35
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
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Gliese 422 system structure

Gliese 422
Gliese 422 b 0.11 AU 11.1 M⊕ 20.1 days

More about Gliese 422

Temperature on its surface is around 3501 K (3228 °C), which is about 61 % of Sun's temperature.
       Gliese 422 can be found in southern celestial hemisphere, however it is too dim to be seen with the naked eye or even a small telescope. 
Other designations of this star
HD 304043, LHS 40, GJ 422, HIP 55042, HIC 55042, LFT 784, L 192-72, LTT 4167, 2MASS J11160018-5732513, Innes star, NLTT 26836, TIC 450545735, TYC 8624-3387-1, WISEA J111557.03-573239.3, Gaia EDR3 5339892367684811520
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External sources
simbad icon
Simbad database (HD 304043)
Astronomical database SIMBAD (the Set of Identifications, Measurements and Bibliography for Astronomical Data)
gaia icon
Gaia database (Gaia EDR3 5339892367684811520)
Archive from the Gaia mission

Frequently Asked Questions

How far is the Gliese 422 system from the Sun?

The Gliese 422 system is 41 light years or 12.7 parsecs from the Sun.

What galaxy is the Gliese 422 star in?

The Gliese 422 is in the Milky Way galaxy just like the Sun.

How many stars are in the Gliese 422 system?

The Gliese 422 is a single star, there are no other known stars in the system.

What type of star is the Gliese 422?

The star Gliese 422 is a Red dwarf star.

What temperature is star Gliese 422?

The star Gliese 422 has an effective temperature of 3501 K. Find out more about the temperature of stars in Stellar guide
Class of stars Red dwarf
Red dwarfs are small, cool stars with surface temperatures of about 2,000–3,800 K, much cooler than the Sun. They usually have 8–50% of the Sun’s mass and shine very faintly, sometimes at just a tiny fraction of the Sun’s brightness. Classified mainly as spectral type M, they are the most common stars in the Milky Way, making up roughly 70–75% of its stellar population.

They fuse hydrogen slowly through the proton–proton chain and are fully convective, which allows them to use their fuel very efficiently. As a result, red dwarfs can live for tens of billions to trillions of years—far longer than the Sun. Many exoplanets orbit red dwarfs, including some in close habitable zones, though strong stellar activity can affect planetary environments.
Closest stars

HD 99279
0.79 M☉ 3.5 ly

Gliese 438
0.4 M☉ 7.1 ly

L 194-11
- 7.6 ly

PM J10382-4933
- 9.6 ly

HD 101581
0.74 M☉ 9.9 ly
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