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Nearby stars catalogue

G 176-34

Star G 176-34

Red dwarf G 176-34 is located 90 light years away from the Sun. It is suspected double or multiple star of spectral class M5V, that has typically about 25 % of solar mass. For now, there are no known exoplanets in this star system.

Sun distance
90 light years

G 176-34

Red dwarf, Spectroscopic binary

Spectral class: M5V

Location +

Right ascension: 11h 24m 59.794s

Declination: 43° 19' 35.983'' (northern hemisphere)

Parallax: 36.046

Sun distance: 90.482 ly | 27.7 pc

Basic characteristic

Mass: 20 % 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 G 176-34

Nearby star G 176-34 is a main sequence star that fuses hydrogen atoms into helium.

       G 176-34 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 DR3 771803119125632896

External sources

Simbad database (G 176-34)

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

Gaia database (Gaia DR3 771803119125632896)

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

UCAC4 671-055873	-	1.3 ly
G 176-8	-	7.3 ly
PM J11075+4345	-	8.1 ly
LSPM J1153+4302	-	8.4 ly
LP 214-23	-	8.6 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.

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.