★ Star V371 Orionis | Nearby stars catalogue

Red dwarf V371 Orionis is located 51.5 light years away from the Sun. It is a single flare star of spectral class M3.0V, that has typically about 25 % of solar mass. For now, there are no known exoplanets in this system.

V371 Orionis

Red dwarf (spectral class M3.0V)

flare star

Mass: 0.35 M Sun (estimate)

Size: 0.38 R Sun (estimate)

Apparent magnitude (V): 11.49

(No known exoplanets yet)

Photometry

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 V371 Orionis

      Nearby star V371 Orionis 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
V* V371 Ori, GJ 9183, Gliese 9183, Gaia EDR3 3223516063958808064

External sources

Sources

Simbad database (V* V371 Ori)

Gaia database (Gaia EDR3 3223516063958808064)

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

Distance (Light Years)		Mass (Solar mass)


5.6	HD 34673	0 M_☉

6.4	LSPM J0540+0854	0 M_☉

6.5	HD 38858	0.89 M_☉

7.5	HD 34673B	0 M_☉

8.7	WISE 0513+0608	0 M_☉

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