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2MASS J22355244+0418563
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Star 2MASS J22355244+0418563

Brown dwarf 2MASS J22355244+0418563 is located 92 light years away from the Sun. It is a single star of spectral class L3, 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
92 light years

2MASS J22355244+0418563

Spectral class: L3

Location +

Ascension iconRight ascension: 22h 35m 52.146s
Declination iconDeclination: 4° 18' 53.776'' (equatorial region)
Parallax iconParallax: 35.429
Distance iconSun distance: 92.059 ly | 28.2 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

radius icon
Size: 10 % R Sun
| 1.1 R Jupiter
(estimate)
+
Star size
Radius of the star 2MASS J22355244+0418563 is not known. Its estimated value based on other similar stars is about 10 % 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 iconTemperature: 2000 K
 (estimate)
+
Star temperature
Surface temperature of 2MASS J22355244+0418563 is estimated to be 2000 K, which is 35 % 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

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 J22355244+0418563 system structure

2MASS J22355244+0418563

More about 2MASS J22355244+0418563

       2MASS J22355244+0418563 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 2705646366448978048
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External sources
simbad icon
Simbad database (2MASS J22355244+0418563)
Astronomical database SIMBAD (the Set of Identifications, Measurements and Bibliography for Astronomical Data)
gaia icon
Gaia database (Gaia DR3 2705646366448978048)
Archive from the Gaia mission

Frequently Asked Questions

How far is the 2MASS J22355244+0418563 system from the Sun?

The 2MASS J22355244+0418563 system is 92 light years or 28.2 parsecs from the Sun.

What galaxy is the 2MASS J22355244+0418563 star in?

The 2MASS J22355244+0418563 is in the Milky Way galaxy just like the Sun.

How many stars are in the 2MASS J22355244+0418563 system?

The 2MASS J22355244+0418563 is a single star, there are no other known stars in the system.

What type of star is the 2MASS J22355244+0418563?

The star 2MASS J22355244+0418563 is a Brown dwarf star.

What temperature is the 2MASS J22355244+0418563?

The primary in the 2MASS J22355244+0418563 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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3. 11. 2026
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TOI-2298 b is about three times Earth’s size and circles its orange dwarf star inside the star’s conservative habitable zone, but uncertain orbits can make such labels misleading. New studies also examine the dust around HD 100546, a possible giant planet around HD 156295, a changing planetary orbit, and how computer models interpret exoplanet atmospheres.
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