ε Cephei (epsilon Cephei)
ε Cephei is a variable and double hypergiant star in the constellation of Cepheus.
ε Cephei visual magnitude is 4.19. Because of its moderate brightness, ε Cephei should be easily visible from locations with dark skies, while it can be barely visible, or not visible at all, from skies affected by light pollution.
The proper motion of ε Cephei is 0.447 arcsec per year in Right Ascension and 0.048 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.
Key facts about ε Cephei
Celestial coordinates and finder chart of ε Cephei
ε Cephei 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 ε Cephei are provided in the following table:
The simplified sky map below shows the position of ε Cephei in the sky:
Visibility of ε Cephei from your location
ε Cephei (epsilon Cephei) is circumpolar and transits at 11:43 UTC (altitude: 84.4°)
Distance of ε Cephei from the Sun and relative movement
ε Cephei is distant 83.89 light years from the Sun and it is moving towards the Sun at the speed of 1 kilometers per second.
Spectral properties of ε Cephei
ε Cephei belongs to spectral class F0 and has a luminosity class of IV corresponding to a hypergiant star.
The red dot in the diagram below shows where ε Cephei is situated in the Hertzsprung–Russell diagram.
ε Cephei star system properties
ε Cephei is a visual double star which can be observed with the help of small or medium telescopes. The table below shows key information about the ε Cephei double sysyem: