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Nearby stars catalogue

SDSS J110142.86+172137.5

Star SDSS J110142.86+172137.5

White dwarf SDSS J110142.86+172137.5 is located 94 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.

Sun distance
94 light years

SDSS J110142.86+172137.5

White dwarf, High proper motion star

Location +

Right ascension: 11h 1m 42.562s

Declination: 17° 21' 33.898'' (equatorial region)

Parallax: 34.668

Sun distance: 94.08 ly | 28.8 pc

Basic characteristic

Photometry

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 SDSS J110142.86+172137.5

       SDSS J110142.86+172137.5 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 DR3 3982007636324256000

External sources

Simbad database (SDSS J110142.86+172137.5)

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

Gaia database (Gaia DR3 3982007636324256000)

Archive from the Gaia mission

Closest stars

HD 96692	-	4.3 ly
LSPM J1108+1545	-	4.5 ly
LP 431-32	-	4.5 ly
LP 374-4	-	6.9 ly
L 1258-39	-	10.5 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.

Fresh and validated

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