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2MASS J11151597+1937266
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Star 2MASS J11151597+1937266

Brown dwarf 2MASS J11151597+1937266 is located 147 light years away from the Sun. It is a single star of spectral class L2γ, 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
147 light years

2MASS J11151597+1937266

Spectral class: L2γ

Location +

Ascension iconRight ascension: 11h 15m 15.899s
Declination iconDeclination: 19° 37' 26.179'' (equatorial region)
Parallax iconParallax: 22.121
Distance iconSun distance: 147.441 ly | 45.2 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: 6 % M Sun
| 62.9 M Jupiter
 (estimate)
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Star mass
The estimated mass of the star 2MASS J11151597+1937266 is about 6 % of the Sun's mass, or approximately 62.9 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
radius icon
Size: 15.4 % R Sun
| 1.5 R Jupiter
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Star size
Radius of the star 2MASS J11151597+1937266 is 0.154 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: 1816 K | 0.31 T Sun
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Star temperature
Surface temperature of 2MASS J11151597+1937266 is 1816 K, which is 31 % 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 J11151597+1937266 system structure

2MASS J11151597+1937266

More about 2MASS J11151597+1937266

Brown dwarf 2MASS J11151597+1937266 is approximately 20 % of the size of Sun and temperature on its surface is around 1816 K (1543 °C), which is about 31 % of Sun's temperature.
       2MASS J11151597+1937266 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 3990192705824438144
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Frequently Asked Questions

How far is the 2MASS J11151597+1937266 system from the Sun?

The 2MASS J11151597+1937266 system is 147 light years or 45.2 parsecs from the Sun.

What galaxy is the 2MASS J11151597+1937266 star in?

The 2MASS J11151597+1937266 is in the Milky Way galaxy just like the Sun.

How many stars are in the 2MASS J11151597+1937266 system?

The 2MASS J11151597+1937266 is a single star, there are no other known stars in the system.

What type of star is the 2MASS J11151597+1937266?

The star 2MASS J11151597+1937266 is a Brown dwarf star.

What temperature is star 2MASS J11151597+1937266?

The star 2MASS J11151597+1937266 has an effective temperature of 1816 K. 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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26. 10. 2026
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A puzzling mass mismatch in the supergiant HD 80077 hints that massive stars may evolve in ways current models cannot fully explain. The latest research also explores how a neutron star’s tilt changes its X-ray light, detects stellar rhythms in infrared observations, and maps cloudy and clear regions on a distant giant planet.
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