Magnitude 3.95 Apparent magnitude (V) 3.95 | ||
Similar Chi Cassiopeiae, Lambda Cassiopeiae, Tau Cassiopeiae, Psi Cassiopeiae, Sigma Cassiopeiae | ||
50 Cassiopeiae is a star in the constellation Cassiopeia. In the past, it had been misidentified as a suspected nebula, and given the number NGC 771.
50 Cassiopeiae is a white A-type main sequence dwarf with an apparent magnitude of +3.95. It is approximately 162.1 light years from Earth. It is a suspected variable star with a very small amplitude.
References
50 Cassiopeiae Wikipedia(Text) CC BY-SA