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Nearby stars catalogue

CX Comae Berenices

Star CX Comae Berenices

Red dwarf CX Comae Berenices is located 87 light years away from the Sun. It is a single flare star of spectral class M4.5, that has typically about 25 % of solar mass. For now, there are no known exoplanets in this star system.

Sun distance
87 light years

CX Comae Berenices

Red dwarf, flare star

Spectral class: M4.5

Location +

Right ascension: 12h 26m 57.48s

Declination: 27° 0' 49.734'' (northern hemisphere)

Parallax: 37.636

Sun distance: 86.66 ly | 26.6 pc

Basic characteristic

Mass: 30 % M Sun

(estimate)

Size: 60 % 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 CX Comae Berenices

       CX Comae Berenices 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
V* CX Com, Gaia DR3 4009083969152655872

External sources

Simbad database (V* CX Com)

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

Gaia database (Gaia DR3 4009083969152655872)

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

HD 108421	-	2.7 ly
TIC 141274365	-	5.2 ly
Wolf 409	-	5.3 ly
G 59-7	-	6.1 ly
LP 320-359	-	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.