34 Persei
34 Persei is a double main-sequence star of spectral class B3 in the constellation of Perseus.
34 Persei visual magnitude is 4.67. Because of its moderate brightness, 34 Persei is easily visible to the naked eye from locations with dark skies, while it might be barely visible, or not visible at all, from light-polluted skies.

Celestial Coordinates
Apparent
J2000
Galactic Coordinates
Finder Chart

Magnitude, Color, Spectral Class
The red dot in the diagram below shows where 34 Persei is situated in the HertzsprungāRussell diagram.

Star System Properties
34 Persei is a visual double star which can be observed with the help of large telescopes. The table below shows key information about the 34 Persei double sysyem:
Distance, Radial Speed, Proper Motion
34 Persei is distant 558.22 light years from the Sun and it is moving towards the Sun at the speed of 2 kilometers per second.
Alternative Designations
Visibility from Your Location
34 Persei is circumpolar and transits at 09:27 UTC (altitude: 88.1°)