Coordinates: 
04h 31m 11.52059s, +58° 58′ 37.4806″
Stein 2051 (Gliese 169.1, G 175-034, LHS 26/27) is a nearby binary star system, containing a red dwarf (component A) and a degenerate star (white dwarf) (component B), located in constellation Camelopardalis at 18.1 ly from Earth. The brighter of this two stars is A (red dwarf), but the more massive is component B (white dwarf). Stein 2051 is the nearest system of Red Dwarf and White Dwarf type.[note 1]
External links [edit]
- ^ 40 Eridani BC is also a system composed of a red dwarf and white dwarf (component B is a white dwarf, and component C is a red dwarf), and located closer (at 16.25 light-years), however, it is not a separate star system, but a subsystem of the 40 Eridani triple star system.
References [edit]
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- Sirius (8.60 ± 0.04 ly; 2 stars)
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- Altair (16.73 ± 0.05 ly; 1 star)
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- Vega (25.04 ± 0.07 ly; 1 star)
- Fomalhaut (25.13 ± 0.09 ly; 1 star, 1 planet: b)
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In left column are stellar classes of primary members of star systems. Bold are systems containing at least one component with absolute magnitude of +8.5 or brighter. Italic are systems without known trigonometric parallax.
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04h 31m 11.52059s, +58° 58′ 37.4806″
