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Nearby stars catalogue

BD+45 4188

Star BD+45 4188

Red dwarf BD+45 4188 is located 78 light years away from the Sun. It is a single star of spectral class M0.5Ve, that has typically about 25 % of solar mass. For now, there are no known exoplanets in this star system.

Sun distance
78 light years

BD+45 4188

Red dwarf, High proper motion star

Spectral class: M0.5Ve

Location +

Right ascension: 23h 18m 18.447s

Declination: 46° 17' 23.598'' (northern hemisphere)

Parallax: 42.04

Sun distance: 77.583 ly | 23.8 pc

Basic characteristic

Mass: 60 % 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 BD+45 4188

Nearby star BD+45 4188 is a main sequence star that fuses hydrogen atoms into helium.

       BD+45 4188 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 1941217160713765376

External sources

Simbad database (BD+45 4188)

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

Gaia database (Gaia EDR3 1941217160713765376)

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

UCAC3 272-282107	-	2.2 ly
HD 218868	-	2.2 ly
UPM J2325+4717	-	4.2 ly
UCAC4 673-120972	-	4.6 ly
WISE J233527.07+451140.9	-	5.5 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.