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Nearby stars catalogue

LSPM J0755+5257

Star LSPM J0755+5257

Red dwarf LSPM J0755+5257 is located 78 light years away from the Sun. It is a single star of spectral class M3.60, that has typically about 25 % of solar mass. For now, there are no known exoplanets in this star system.

Sun distance
78 light years

LSPM J0755+5257

Red dwarf, High proper motion star

Spectral class: M3.60

Location +

Right ascension: 7h 55m 12.342s

Declination: 52° 57' 53.162'' (northern hemisphere)

Parallax: 41.559

Sun distance: 78.481 ly | 24.1 pc

Basic characteristic

Mass: 40 % M Sun

(estimate)

Size: 100 % 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 J0755+5257

       LSPM J0755+5257 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 984602805724340608

External sources

Simbad database (LSPM J0755+5257)

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

Gaia database (Gaia EDR3 984602805724340608)

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

LP 123-75	-	5.2 ly
LP 89-187	-	6 ly
2MASS J07483900+5338533	-	6.7 ly
G 193-65	-	7 ly
EGGR 344	-	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.

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.