54 Persei is a double giant star in the constellation of Perseus.
54 Persei visual magnitude is 4.93. Because of its moderate brightness, 54 Persei should be easily visible from locations with dark skyes, while it can be barely visible, or not visible at all, from skyes affected by light pollution.
The table below summarizes the key facts about 54 Persei:
Celestial coordinates and finder chart of 54 Persei
54 Persei is situated north of the celestial equator, as such, it is more easily visible from the northern hemisphere. Celestial coordinates for the J2000 equinox as well as galactic coordinates of 54 Persei are provided in the following table:
The simplified sky map below shows the position of 54 Persei in the sky:
Visibility of 54 Persei from your location
Digitized Sky Survey image of 54 Persei
The image below is a photograph of 54 Persei from the Digitized Sky Survey 2 (DSS2 - see the credits section) taken in the red channel. The area of sky represented in the image is 0.5x0.5 degrees (30x30 arcmins). The proper motion of 54 Persei is -0.025 arcsec per year in Right Ascension and -0.005 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of 54 Persei from the Sun and relative movement
54 Persei is distant 226.07 light years from the Sun and it is moving towards the Sun at the speed of 27 kilometers per second.
Spectral properties of 54 Persei
54 Persei belongs to spectral class G8 and has a luminosity class of III corresponding to a giant star.
The red dot in the diagram below shows where 54 Persei is situated in the Hertzsprung–Russell diagram.
54 Persei star system properties
54 Persei is a visual double star which can be observed only with the help of very large telescopes. The table below shows key information about the 54 Persei double sysyem: