HR567 is a double hypergiant star in the constellation of Cassiopeia.
HR567 visual magnitude is 5.26. Because of its reltive faintness, HR567 should be visible only from locations with dark skyes, while it is not visible at all from skyes affected by light pollution.
The table below summarizes the key facts about HR567:
Celestial coordinates and finder chart of HR567
HR567 is situated close to the northern celestial pole and, as such, it is visible for most part of the year from the northern hemisphere. Celestial coordinates for the J2000 equinox as well as galactic coordinates of HR567 are provided in the following table:
The simplified sky map below shows the position of HR567 in the sky:
Visibility of HR567 from your location
HR567 is circumpolar and transits at 16:49 UTC (altitude: 76.9°)
Digitized Sky Survey image of HR567
The image below is a photograph of HR567 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 HR567 is 0.033 arcsec per year in Right Ascension and -0.02 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR567 from the Sun and relative movement
HR567 is distant 256.90 light years from the Sun and it is moving far from the Sun at the speed of 5 kilometers per second.
Spectral properties of HR567
HR567 belongs to spectral class A0 and has a luminosity class of V corresponding to a hypergiant star.
The red dot in the diagram below shows where HR567 is situated in the Hertzsprung–Russell diagram.
HR567 star system properties
HR567 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 HR567 double sysyem: