Magnitude 4.32 Apparent magnitude (V) 4.32 | ||
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Nu Serpentis (ν Ser, ν Serpentis) is a binary star in the constellation Serpens. It is approximately 203 light years from Earth.
The primary component, Nu Serpentis A, is a white A-type main sequence dwarf with an apparent magnitude of +4.32. It is separated from Nu Serpentis B, a magnitude +9.4 companion, by 46 arcseconds.
References
Nu Serpentis Wikipedia(Text) CC BY-SA