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G 32-5
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Star G 32-5

Red dwarf G 32-5 is located 40 light years away from the Sun. It is a single star of spectral class M3V, that has 24 % of solar mass. There is at least one exoplanet in this system.
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Sun distance
40 light years
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G 32-5

Red dwarf, High proper motion star
Spectral class: M3V

Location +

Ascension iconRight ascension: 0h 15m 49.928s
Declination iconDeclination: 13° 33' 27.587'' (equatorial region)
Parallax iconParallax: 82.194
Distance iconSun distance: 39.681 ly | 12.2 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: 24.1 % M Sun
| 253 M Jupiter
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Star mass
Mass of the star G 32-5 is 0.2414 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
radius icon
Size: 26 % R Sun
| 2.6 R Jupiter
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Star size
Radius of the star G 32-5 is 0.2617 solar radii.

The size of a star refers to its radius — the distance from its center to its surface. Star size is usually measured in solar radii (R☉), where 1 solar radius equals approximately 696,000 kilometers. Depending on their type and life stage, stars can be much smaller or larger than the Sun... icon More about Star size in StellarGuide
temperature icon
Temperature: 3296 K | 0.57 T Sun
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Star temperature
Surface temperature of G 32-5 is 3296 K, which is 57 % 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): 12.6
Magnitude iconAbsolute magnitude (V): 12.2
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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G 32-5 system structure

 G 32-5
G 32-5 b 0.07 AU 0.7 M⊕ 0.9 R⊕ 12.8 days

More about G 32-5

Nearby star G 32-5 is a main sequence star that fuses hydrogen atoms into helium. It is approximately 30 % of the size of Sun and temperature on its surface is around 3296 K (3023 °C), which is about 57 % of Sun's temperature.
       G 32-5 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
Gliese 12, GJ 12, TOI-6251, LHS 1050, TIC 52005579, LP 464-42, WISEA J001549.70+133325.8, 2MASS J00154919+1333218, G 30-55, , Gaia EDR3 2768048564768256512
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External sources
icon study
simbad icon
Simbad database (G 32-5)
Astronomical database SIMBAD (the Set of Identifications, Measurements and Bibliography for Astronomical Data)
gaia icon
Gaia database (Gaia EDR3 2768048564768256512)
Archive from the Gaia mission

Frequently Asked Questions

How far is the G 32-5 system from the Sun?

The G 32-5 system is 40 light years or 12.2 parsecs from the Sun.

What galaxy is the G 32-5 star in?

The G 32-5 is in the Milky Way galaxy just like the Sun.

How many stars are in the G 32-5 system?

The G 32-5 is a single star, there are no other known stars in the system.

What type of star is the G 32-5?

The star G 32-5 is a Red dwarf star.

What temperature is star G 32-5?

The star G 32-5 has an effective temperature of 3296 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

 54 Piscium
 0.76 M☉ 7.2 ly

G 32-35
 - 8.5 ly

LP 463-23
 - 8.6 ly

WISEA J2354+0240
 - 8.8 ly

G 129-47
 - 8.9 ly
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