50 Persei
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Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
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Constellation | Perseus |
Right ascension | 04h 08m 36.61660s [1] |
Declination | +38° 02′ 23.0488″ [1] |
Spectral type | F7V |
50 Persei is a star in the constellation Perseus. Its apparent magnitude is 5.50. Located around 21.00 parsecs (68.5 ly) distant, it is a White main-sequence star of spectral type F7V,[1] a star that is currently fusing its core hydrogen. The star is an RS Canum Venaticorum variable,[1] meaning that it is a close binary star whose components have star-spots, which cause variations in brightness.
References
- ↑ 1.0 1.1 1.2 1.3 "14 Persei". SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg. Retrieved 31 December 2013.
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