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Nearby stars catalogue

L 536-155

Star L 536-155

White dwarf L 536-155 is located 90 light years away from the Sun. It is a single star of spectral class DAH D, that has typically about 60 % of solar mass. For now, there are no known exoplanets in this star system.

Sun distance
90 light years

L 536-155

White dwarf, High proper motion star

Spectral class: DAH D

Location +

Right ascension: 10h 19m 46.89s

Declination: -34° 2' 19.441'' (southern hemisphere)

Parallax: 36.301

Sun distance: 89.847 ly | 27.5 pc

Basic characteristic

Photometry

Apparent magnitude (V): 16.5

Absolute magnitude (V): 14.3

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 L 536-155

       L 536-155 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
2MASS J10194735-3402219, WISE J101947.04-340220.2, TIC 71407717, Gaia DR3 5446784345474819968

External sources

Simbad database (L 536-155)

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

Gaia database (Gaia DR3 5446784345474819968)

Archive from the Gaia mission

Closest stars

WT 2473	-	4.8 ly
CD-35 6480	-	5 ly
PM J10107-3046	-	7 ly
CD-30 8159	-	7.4 ly
SIPS J1018-2909	-	7.8 ly

3D map of stellar neighborhood
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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.