NU SERPENTIS


'Nu Serpentis' (ν Ser / ν Serpentis) is a binary star in the constellation Serpens. It is approximately 193 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 +8.4 companion, by 46 arcseconds.

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