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Nearby stars catalogue

CD-45 13383

Star CD-45 13383

Red dwarf CD-45 13383 is located 81 light years away from the Sun. It is a single star of spectral class M1V, that has typically about 25 % of solar mass. For now, there are no known exoplanets in this star system.

Sun distance
81 light years

CD-45 13383

Red dwarf, High proper motion star

Spectral class: M1V

Location +

Right ascension: 19h 42m 52.71s

Declination: -45° 4' 57.386'' (southern hemisphere)

Parallax: 40.473

Sun distance: 80.586 ly | 24.7 pc

Basic characteristic

Mass: 50 % M Sun

(estimate)

Size: 50 % R Sun

(estimate)

Photometry

Apparent magnitude (V): 10

Absolute magnitude (V): 8.1

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 CD-45 13383

Nearby star CD-45 13383 is a main sequence star that fuses hydrogen atoms into helium.

       CD-45 13383 can be found in southern celestial hemisphere, you cannot see it with naked eye, but you can observe this star with basic telescope. The star is also observable from Northern America, Europe and Asia.

Other designations of this star
Gaia EDR3 6684697235617251200

External sources

Simbad database (CD-45 13383)

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

Gaia database (Gaia EDR3 6684697235617251200)

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

SCR J1936-4816	-	4.8 ly
UCAC4 221-179366	-	5.1 ly
Gaia DR2 6689574432978156160	-	5.4 ly
UCAC3 94-383364	-	5.7 ly
SSSPM J1926-4311	-	5.8 ly

3D map of stellar neighborhood
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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.

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.