Star G 86-27

Red dwarf G 86-27 is located 91 light years away from the Sun. It is a single star, that has typically about 25 % of solar mass. For now, there are no known exoplanets in this star system.

G 86-27

Red dwarf, High proper motion star

Location

Right ascension: 5h 10m 32.162s

Declination: 31° 17' 31.813'' (northern hemisphere)

Parallax: 35.685

Sun distance: 91.398 ly | 28 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 86-27

       G 86-27 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 180503800659357312

External sources

Simbad database (G 86-27)

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

Gaia database (Gaia DR3 180503800659357312)

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

G 85-49	-	7 ly
HD 31000	-	10.3 ly
HD 33632	1.1 M☉	10.8 ly
UPM J0516+2445	-	10.8 ly
LSPM J0533+3740	-	13.6 ly

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