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Nearby stars catalogue

LSPM J1557+0901

Star LSPM J1557+0901

Red dwarf LSPM J1557+0901 is located 62 light years away from the Sun. It is a single star of spectral class M4.0V, that has typically about 25 % of solar mass. For now, there are no known exoplanets in this star system.

Sun distance
62 light years

LSPM J1557+0901

Red dwarf, High proper motion star

Spectral class: M4.0V

Location +

Right ascension: 15h 57m 48.427s

Declination: 9° 1' 7.613'' (equatorial region)

Parallax: 52.277

Sun distance: 62.39 ly | 19.1 pc

Basic characteristic

Mass: 30 % M Sun

(estimate)

Size: 30 % R Sun

(estimate)

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 J1557+0901

Nearby star LSPM J1557+0901 is a main sequence star that fuses hydrogen atoms into helium.

       LSPM J1557+0901 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 4454532237354157568

External sources

Simbad database (LSPM J1557+0901)

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

Gaia database (Gaia DR3 4454532237354157568)

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

39 Serpentis	-	6.3 ly
BD+11 2874	-	6.9 ly
2MASS J1615+0546	-	7.2 ly
G 137-24	-	7.4 ly
2MASS J1534+1219	-	7.8 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.