Star Ross 52 B

Red dwarf Ross 52 B is located 37.8 light years away from the Sun. It is a single star of spectral class M4, that has typically about 25 % of solar mass. For now, there are no known exoplanets in this system.

Red dwarfs are small reddish stars, it is by far the most common type of star in solar neighborhood.
Sun distance: 37.8 light years.
(Position of this star is derived from Gaia mission data.)
Ross 52 B
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Red dwarf
spectral class M4

0.25 solar masses (estimate)
0.28 solar radii (estimate)
(No known exoplanets yet)
Other designations of this star
Gaia EDR3 1266092694562422912
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Closest stars
Distance
(Light Years)
Star name Mass
(Solar mass)
Planets
0.5
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Ross 52 0 M
0 M
2.9
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V* DE Boo 0 M
3
part of star image
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TVLM 513-46 0.09 M
1
4.6
part of star image
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V* OT Ser 0 M
6.1
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Ross 508 0 M
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