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Nearby stars catalogue

LSPM J1305+1934

Star LSPM J1305+1934

Red dwarf LSPM J1305+1934 is located 90 light years away from the Sun. It is a single star of spectral class M6.5, that has typically about 25 % of solar mass. For now, there are no known exoplanets in this star system.

Sun distance
90 light years

LSPM J1305+1934

Red dwarf, High proper motion star

Spectral class: M6.5

Location +

Right ascension: 13h 5m 36.393s

Declination: 19° 35' 4.856'' (equatorial region)

Parallax: 36.135

Sun distance: 90.26 ly | 27.7 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 LSPM J1305+1934

       LSPM J1305+1934 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 3941419679982061824

External sources

Simbad database (LSPM J1305+1934)

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

Gaia database (Gaia DR3 3941419679982061824)

Archive from the Gaia mission

Class of stars Red dwarf

Red dwarfs are small, relatively cool, reddish stars. They are by far the most common type of star in the solar neighborhood. Their mass typically ranges from about 8% to 50% of the Sun's mass.

Closest stars

G 63-3	-	5.3 ly
MCC 686	-	6.5 ly
Gaia DR2 3941497741011628672	-	6.5 ly
KX Comae Berenices	-	7 ly
G 61-48	-	7 ly

3D map of stellar neighborhood
List of all nearby stars

About Stellar Catalog

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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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