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Nearby stars catalogue

LEHPM 2-801

Star LEHPM 2-801

Red dwarf LEHPM 2-801 is located 70 light years away from the Sun. It is a single star, that has typically about 25 % of solar mass. For now, there are no known exoplanets in this star system.

Sun distance
70 light years

LEHPM 2-801

Red dwarf, High proper motion star

Location +

Right ascension: 21h 22m 16.866s

Declination: -43° 14' 8.482'' (southern hemisphere)

Parallax: 46.27

Sun distance: 70.489 ly | 21.6 pc

Basic characteristic

Mass: 30 % M Sun

(estimate)

Size: 30 % R Sun

(estimate)

Photometry

Apparent magnitude (V): 13.4

Absolute magnitude (V): 11.7

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 LEHPM 2-801

       LEHPM 2-801 can be found in southern 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 6577290140883225984

External sources

Simbad database (LEHPM 2-801)

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

Gaia database (Gaia EDR3 6577290140883225984)

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

L 353-143	-	4.8 ly
HD 199288	0.82 M☉	5.6 ly
APMPM J2127-3844	-	6.6 ly
HD 202628	1.1 M☉	7.2 ly
HD 203985	-	7.2 ly

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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.

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