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Gaia EDR3 5733429157137237760
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Star Gaia EDR3 5733429157137237760

Brown dwarf Gaia EDR3 5733429157137237760 is located 57 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
57 light years
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Gaia EDR3 5733429157137237760

Brown dwarf
Spectral class: L1.5

Location +

Ascension iconRight ascension: 8h 47m 28.893s
Declination iconDeclination: -15° 32' 40.573'' (equatorial region)
Parallax iconParallax: 57.511
Distance iconSun distance: 56.712 ly | 17.4 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 Gaia EDR3 5733429157137237760 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)
+
Star temperature
Surface temperature of Gaia EDR3 5733429157137237760 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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Gaia EDR3 5733429157137237760 system structure

 Gaia EDR3 5733429157137237760

More about Gaia EDR3 5733429157137237760

       Gaia EDR3 5733429157137237760 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 5733429157137237760
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External sources
simbad icon
Simbad database (SIPS J0847-1532)
Astronomical database SIMBAD (the Set of Identifications, Measurements and Bibliography for Astronomical Data)
gaia icon
Gaia database (Gaia EDR3 5733429157137237760)
Archive from the Gaia mission

Frequently Asked Questions

How far is the Gaia EDR3 5733429157137237760 system from the Sun?

The Gaia EDR3 5733429157137237760 system is 57 light years or 17.4 parsecs from the Sun.

What galaxy is the Gaia EDR3 5733429157137237760 star in?

The Gaia EDR3 5733429157137237760 is in the Milky Way galaxy just like the Sun.

How many stars are in the Gaia EDR3 5733429157137237760 system?

The Gaia EDR3 5733429157137237760 is a single star, there are no other known stars in the system.

What type of star is the Gaia EDR3 5733429157137237760?

The star Gaia EDR3 5733429157137237760 is a Brown dwarf star.

What temperature is the Gaia EDR3 5733429157137237760?

The primary in the Gaia EDR3 5733429157137237760 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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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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