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DENIS J075116.4-253043
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Star DENIS J075116.4-253043

Brown dwarf DENIS J075116.4-253043 is located 58 light years away from the Sun. It is a single star of spectral class L1.5, 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
58 light years

DENIS J075116.4-253043

Spectral class: L1.5

Location +

Ascension iconRight ascension: 7h 51m 15.359s
Declination iconDeclination: -25° 30' 40.707'' (southern hemisphere)
Parallax iconParallax: 56.416
Distance iconSun distance: 57.812 ly | 17.7 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

radius icon
Size: 10 % R Sun
| 1 R Jupiter
(estimate)
+
Star size
Radius of the star DENIS J075116.4-253043 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: 2200 K
 (estimate)
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Star temperature
Surface temperature of DENIS J075116.4-253043 is estimated to be 2151 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): -1.2
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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DENIS J075116.4-253043 system structure

DENIS J075116.4-253043

More about DENIS J075116.4-253043

       DENIS J075116.4-253043 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 EDR3 5602408602804816768
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External sources
simbad icon
Simbad database (DENIS J075116.4-253043)
Astronomical database SIMBAD (the Set of Identifications, Measurements and Bibliography for Astronomical Data)
gaia icon
Gaia database (Gaia EDR3 5602408602804816768)
Archive from the Gaia mission

Frequently Asked Questions

How far is the DENIS J075116.4-253043 system from the Sun?

The DENIS J075116.4-253043 system is 58 light years or 17.7 parsecs from the Sun.

What galaxy is the DENIS J075116.4-253043 star in?

The DENIS J075116.4-253043 is in the Milky Way galaxy just like the Sun.

How many stars are in the DENIS J075116.4-253043 system?

The DENIS J075116.4-253043 is a single star, there are no other known stars in the system.

What type of star is the DENIS J075116.4-253043?

The star DENIS J075116.4-253043 is a Brown dwarf star.

What temperature is the DENIS J075116.4-253043?

The primary in the DENIS J075116.4-253043 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.
Closest stars

SCR J0753-2524
- 0.7 ly

HIP 38594
0.61 M☉ 0.7 ly

HD 65486
- 2.9 ly

UPM J0730-2831
- 5.8 ly

Gaia DR2 5715492411643646976
- 5.8 ly
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stellar brief logoStellar Brief

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30. 10. 2026
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The early architecture of planetary systems may be set at birth: a study of Sun-like stars found similar rates of star-planet misalignment across different stages of development. Other findings trace how water and carbon dioxide ice fade around young stars, why white-dwarf debris resists breaking into tiny pieces, and why a reported planet around Gliese 48 remains unconfirmed.
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