do not follow here
Stellar Catalog
more icon
Nearby stars catalogue
more icon
G 209-38
more icon

Star G 209-38

Red dwarf G 209-38 is located 53 light years away from the Sun. It is a single star of spectral class M3.5, that has typically about 25 % of solar mass. For now, there are no known exoplanets in this star system.
Sun distance
53 light years

G 209-38

Red dwarf (spectral class M3.5)

Location

Ascension iconRight ascension: 20h 36m 46.275s
Declination iconDeclination: 38° 50' 30.264'' (northern hemisphere)
Parallax iconParallax: 61.132
Distance iconSun distance: 53.353 ly | 16.4 pc

Basic characteristic

icon weight
Mass: 30 % M Sun | 303.8 M Jupiter (estimate)
radius icon
Size: 30 % R Sun | 3.2 R Jupiter (estimate)
(No known exoplanets yet)

Photometry

Magnitude iconApparent magnitude (V): 13.4
Magnitude iconAbsolute magnitude (V): 12.3
5
10
15
20
25
30
35
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
Absolute stellar magnitude in different parts of the electromagnetic spectrum from infrared (K band) to ultraviolet (U band).
More about G 209-38
      G 209-38 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 2063967910147595008
External sources
simbad icon
Simbad database (G 209-38)
Astronomical database SIMBAD (the Set of Identifications, Measurements and Bibliography for Astronomical Data)
gaia icon
Gaia database (Gaia EDR3 2063967910147595008)
Archive from the Gaia mission
Class of stars Red dwarf
Red dwarfs are small reddish stars, that are by far the most common type of star in solar neighborhood. Their mass is usually between 10 and 50 % of solar mass.
Closest stars

Ross 188
- 3.3 ly

EGGR 261
- 4.8 ly

G 212-5
- 5.1 ly

LSPM J2049+3336
0.1 M☉ 5.6 ly

BD+40 883
- 6 ly
3D map of stellar neighborhood
List of all nearby stars
Get your next news from nearby stars
This is a new project, and partly still in development. There will be soon more information and functions. We would love your support on social media.