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PM J13332-6751
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Star PM J13332-6751

White dwarf PM J13332-6751 is located 86 light years away from the Sun. It is a single star, 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
86 light years
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PM J13332-6751

White dwarf, High proper motion star

Location +

Ascension iconRight ascension: 13h 33m 12.551s
Declination iconDeclination: -67° 51' 22.278'' (southern hemisphere)
Parallax iconParallax: 37.982
Distance iconSun distance: 85.870 ly | 26.3 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: 60 % M Sun
| 597.1 M Jupiter
 (estimate)
+
Star mass
The mass of the star PM J13332-6751 is unknown. Based on its other characteristics, it is estimated to be about 60 % 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 iconTemperature: 6500 K
 (estimate)
+
Star temperature
Surface temperature of PM J13332-6751 is estimated to be 6500 K, which is 112 % 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 iconApparent magnitude (V): 17.2
Magnitude iconAbsolute magnitude (V): 15.1
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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PM J13332-6751 system structure

 PM J13332-6751

More about PM J13332-6751

       PM J13332-6751 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 5845312191917620224
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External sources
simbad icon
Simbad database (PM J13332-6751)
Astronomical database SIMBAD (the Set of Identifications, Measurements and Bibliography for Astronomical Data)
gaia icon
Gaia database (Gaia DR3 5845312191917620224)
Archive from the Gaia mission

Frequently Asked Questions

How far is the PM J13332-6751 system from the Sun?

The PM J13332-6751 system is 86 light years or 26.3 parsecs from the Sun.

What galaxy is the PM J13332-6751 star in?

The PM J13332-6751 is in the Milky Way galaxy just like the Sun.

How many stars are in the PM J13332-6751 system?

The PM J13332-6751 is a single star, there are no other known stars in the system.

What type of star is the PM J13332-6751?

The star PM J13332-6751 is a White dwarf star.

What temperature is the PM J13332-6751?

The primary in the PM J13332-6751 system has an effective temperature of K ( °C). Find out more about the temperature of stars in Stellar guide
Possible companions

 L 106-69
 - 0.1 ly
Closest stars

 UPM J1303-6528
 - 6.5 ly

Delta Muscae
 - 7 ly

UPM J1316-7126
 - 8 ly

CD-67 1583
 - 8 ly

UPM J1343-7305
 - 8.4 ly
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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.
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