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Nearby stars catalogue

LP 544-17

Star LP 544-17

Red dwarf LP 544-17 is located 78 light years away from the Sun. It is a single star of spectral class M6, that has typically about 25 % of solar mass. For now, there are no known exoplanets in this star system.

Sun distance
78 light years

LP 544-17

Red dwarf, Low-mass star

Spectral class: M6

Location +

Right ascension: 8h 3m 44.619s

Declination: 8° 26' 56.759'' (equatorial region)

Parallax: 41.808

Sun distance: 78.012 ly | 23.9 pc

Basic characteristic

Mass: 10 % M Sun

(estimate)

Size: 20 % 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 LP 544-17

       LP 544-17 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 3146187071877364992

External sources

Simbad database (LP 544-17)

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

Gaia database (Gaia EDR3 3146187071877364992)

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

PM J08103+0935	-	5.1 ly
LSPM J0804+1116	-	6.1 ly
2MASS J08151407+1030117	-	7.1 ly
PM J08202+0532	-	8.1 ly
LSPM J0805+0417	-	8.2 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.