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Nearby stars catalogue

PM J15589+0417

Star PM J15589+0417

White dwarf PM J15589+0417 is located 73 light years away from the Sun. It is a single star of spectral class DC, that has typically about 60 % of solar mass. For now, there are no known exoplanets in this star system.

Sun distance
73 light years

PM J15589+0417

White dwarf

Spectral class: DC

Location +

Right ascension: 15h 58m 57.665s

Declination: 4° 17' 3.986'' (equatorial region)

Parallax: 44.427

Sun distance: 73.414 ly | 22.5 pc

Basic characteristic

Photometry

Apparent magnitude (V): 16.2

Absolute magnitude (V): 14.4

Absolute stellar magnitude in different parts of the electromagnetic spectrum from infrared (K band) to ultraviolet (U band).

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

More about PM J15589+0417

       PM J15589+0417 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 4425632987265111680

External sources

Simbad database (PM J15589+0417)

Astronomical database SIMBAD (the Set of Identifications, Measurements and Bibliography for Astronomical Data)

Gaia database (Gaia EDR3 4425632987265111680)

Archive from the Gaia mission

Closest stars

Epsilon Serpentis	1.8 M☉	3 ly
PM J16060+0333	-	4.4 ly
Alpha Serpentis	1.7 M☉	5.5 ly
HD 141272	-	5.5 ly
LSPM J1619+0140	-	7.3 ly

3D map of stellar neighborhood
List of all nearby stars

About Stellar Catalog

Working with real data

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

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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Stellar Catalog is continuously updated with new information from research papers. Stellar and planetary data are validated by automatic processes as well as humans.