Nearby stars catalogue < LIVING fUTURE

Star V371 Orionis

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.
Sun distance
51.5 light years
Position of this star is derived from Gaia mission data.
V371 Orionis
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Red dwarf (spectral class M3.0V)
flare star

Mass: 0.35 M Sun | M Jupiter (estimate)
radius icon
Size: 0.38 R Sun (estimate)
Magnitude iconApparent magnitude (V): 11.49
(No known exoplanets yet)
Photometry
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
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 icon Simbad database (V* V371 Ori)
simbad icon Gaia database (Gaia EDR3 3223516063958808064)
Class of stars Red dwarf
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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)
Star name Mass
(Solar mass)
Planets
5.6
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HD 34673 0 M
6.4
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LSPM J0540+0854 0 M
6.5
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HD 38858 0.89 M
7.5
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HD 34673B 0 M
8.7
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WISE 0513+0608 0 M
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v371-orionis