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WD J2141-3300
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Star WD J2141-3300

White dwarf WD J2141-3300 is located 53 light years away from the Sun. It is a single star of spectral class DZAH, that has typically about 60 % of solar mass. For now, there are no known exoplanets in this star system.
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Sun distance
53 light years

WD J2141-3300

Spectral class: DZAH

Location +

Ascension iconRight ascension: 21h 41m 57.344s
Declination iconDeclination: -33° 0' 31.615'' (southern hemisphere)
Parallax iconParallax: 62.070
Distance iconSun distance: 52.546 ly | 16.1 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: 100 % M Sun
| 995.2 M Jupiter
 (estimate)
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Star mass
The mass of the star WD J2141-3300 is unknown. Based on its other characteristics, it is estimated to be about 100 % of the Sun's mass.

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 icon
Temperature: 6870 K | 1.19 T Sun
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Star temperature
Surface temperature of WD J2141-3300 is 6870 K, which is 119 % 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
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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WD J2141-3300 system structure

WD J2141-3300

More about WD J2141-3300

Temperature on its surface is around 6870 K (6597 °C), which is about 119 % of Sun's temperature.
       WD J2141-3300 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 6592315723192176896
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Frequently Asked Questions

How far is the WD J2141-3300 system from the Sun?

The WD J2141-3300 system is 53 light years or 16.1 parsecs from the Sun.

What galaxy is the WD J2141-3300 star in?

The WD J2141-3300 is in the Milky Way galaxy just like the Sun.

How many stars are in the WD J2141-3300 system?

The WD J2141-3300 is a single star, there are no other known stars in the system.

What type of star is the WD J2141-3300?

The star WD J2141-3300 is a White dwarf star.

What temperature is star WD J2141-3300?

The star WD J2141-3300 has an effective temperature of 6870 K. Find out more about the temperature of stars in Stellar guide
Possible companions

L 570-26
0.6 M☉ 0 ly

stellar brief logoStellar Brief

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24. 10. 2026
stellar brief logo
A planet’s helium atmosphere streams ahead of its orbit, while infrared observations reveal the hidden rhythms of its star. New work also shows how neutron-star tilt can reshape X-ray light, traces the past of massive blue supergiants, and maps cloudy and clear zones on the hot Jupiter WASP-43 b.
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exoplanet iconAbout Stellar Catalog

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Working with real data
icon Data in Stellar Catalog come from trusted scientific sources. Primary source is Gaia space telescope mapping the stars in Milky Way. Other sources include research papers, Simbad catalog and Exoplanet.eu database.
Estimated values
icon Objects listed in the Stellar Catalog often have values that are estimates. These estimates are determined using their known characteristics, such as spectral type, brightness across different wavelengths, distance from a star, and other factors.
Fresh and validated
icon Stellar Catalog is continuously updated with new information from research papers. Stellar and planetary data are validated by automatic processes as well as humans.

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