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LSR J0401+5131
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Star LSR J0401+5131

White dwarf LSR J0401+5131 is located 82 light years away from the Sun. It is a single star of spectral class DC8, 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
82 light years
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LSR J0401+5131

White dwarf
Spectral class: DC8

Location +

Ascension iconRight ascension: 4h 1m 2.144s
Declination iconDeclination: 51° 31' 17.238'' (northern hemisphere)
Parallax iconParallax: 39.836
Distance iconSun distance: 81.875 ly | 25.1 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: 60 % M Sun
| 597.1 M Jupiter
 (estimate)
+
Star mass
The mass of the star LSR J0401+5131 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 LSR J0401+5131 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

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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LSR J0401+5131 system structure

 LSR J0401+5131

More about LSR J0401+5131

       LSR J0401+5131 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 EDR3 250862824946594816
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External sources
simbad icon
Simbad database (LSR J0401+5131)
Astronomical database SIMBAD (the Set of Identifications, Measurements and Bibliography for Astronomical Data)
gaia icon
Gaia database (Gaia EDR3 250862824946594816)
Archive from the Gaia mission

Frequently Asked Questions

How far is the LSR J0401+5131 system from the Sun?

The LSR J0401+5131 system is 82 light years or 25.1 parsecs from the Sun.

What galaxy is the LSR J0401+5131 star in?

The LSR J0401+5131 is in the Milky Way galaxy just like the Sun.

How many stars are in the LSR J0401+5131 system?

The LSR J0401+5131 is a single star, there are no other known stars in the system.

What type of star is the LSR J0401+5131?

The star LSR J0401+5131 is a White dwarf star.

What temperature is the LSR J0401+5131?

The primary in the LSR J0401+5131 system has an effective temperature of K ( °C). Find out more about the temperature of stars in Stellar guide
Possible companions

 Ross 25
 - 0.2 ly
Closest stars

 HD 23140
 - 8.7 ly

Ross 23
 - 8.9 ly

Gaia DR3 251476382498509952
 - 9 ly

HD 232781
 - 9.3 ly

LSPM J0343+4554
 - 9.7 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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