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2MASS J23211254-1326282
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Star 2MASS J23211254-1326282

Brown dwarf 2MASS J23211254-1326282 is located 93 light years away from the Sun. It is a single star of spectral class L0.5, that has typically about 4 % of solar mass. For now, there are no known exoplanets in this star system.
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Sun distance
93 light years

2MASS J23211254-1326282

Spectral class: L0.5

Location +

Ascension iconRight ascension: 23h 21m 13.164s
Declination iconDeclination: -13° 26' 30.822'' (equatorial region)
Parallax iconParallax: 35.094
Distance iconSun distance: 92.937 ly | 28.5 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: 8 % M Sun
| 83.8 M Jupiter
 (estimate)
+
Star mass
The estimated mass of the star 2MASS J23211254-1326282 is about 8 % of the Sun's mass, or approximately 83.8 Jupiter 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 iconTemperature: 2200 K
 (estimate)
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Star temperature
Surface temperature of 2MASS J23211254-1326282 is estimated to be 2226 K, which is 38 % 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 iconAbsolute magnitude (V): -2.3
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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2MASS J23211254-1326282 system structure

2MASS J23211254-1326282

More about 2MASS J23211254-1326282

       2MASS J23211254-1326282 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
Gaia DR3 2408845056640573056
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External sources
simbad icon
Simbad database (2MASS J23211254-1326282)
Astronomical database SIMBAD (the Set of Identifications, Measurements and Bibliography for Astronomical Data)
gaia icon
Gaia database (Gaia DR3 2408845056640573056)
Archive from the Gaia mission

Frequently Asked Questions

How far is the 2MASS J23211254-1326282 system from the Sun?

The 2MASS J23211254-1326282 system is 93 light years or 28.5 parsecs from the Sun.

What galaxy is the 2MASS J23211254-1326282 star in?

The 2MASS J23211254-1326282 is in the Milky Way galaxy just like the Sun.

How many stars are in the 2MASS J23211254-1326282 system?

The 2MASS J23211254-1326282 is a single star, there are no other known stars in the system.

What type of star is the 2MASS J23211254-1326282?

The star 2MASS J23211254-1326282 is a Brown dwarf star.

What temperature is the 2MASS J23211254-1326282?

The primary in the 2MASS J23211254-1326282 system has an effective temperature of K ( °C). Find out more about the temperature of stars in Stellar guide
Class of stars Brown dwarf
Brown dwarfs are not really stars, because there is no thermonuclear fusion in their core. These objects are smaller and cooler than stars, but too massive to be considered planets.
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stellar brief logoStellar Brief

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29. 10. 2026
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Weighing potentially habitable planets around Sun-like stars remains surprisingly difficult: a methods test found that precise measurements often require planets weighing about 8 to 10 Earth masses. The latest reports also explore brilliant radio bursts from a rapidly spinning brown dwarf, a possible hotspot on another brown dwarf, and how transit changes can expose a planet that never crosses its star.
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