Nu Serpentis
| This article does not cite any references or sources. (December 2009) |
| Observation data Epoch J2000.0 Equinox J2000.0 |
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| Constellation | Serpens |
| Right ascension | 17h 20m 49.7s |
| Declination | -12° 50' 49" |
| Apparent magnitude (V) | +4.32 |
| Distance | 193 ± 10 ly (59 ± 3 pc) |
| Spectral type | A0/A1V |
| Other designations | |
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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