HR8327 is a double supergiant star in the constellation of Cepheus.
HR8327 visual magnitude is 5.95. Because of its reltive faintness, HR8327 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 HR8327:
Celestial coordinates and finder chart of HR8327
HR8327 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 HR8327 are provided in the following table:
The simplified sky map below shows the position of HR8327 in the sky:
Visibility of HR8327 from your location
HR8327 is circumpolar and transits at 17:20 UTC (altitude: 79.0°)
Digitized Sky Survey image of HR8327
The image below is a photograph of HR8327 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 HR8327 is -0.007 arcsec per year in Right Ascension and -0.002 arcsec per year in Declination and the associated displacement for the next 100000 years is represented with the red arrow.
Distance of HR8327 from the Sun and relative movement
HR8327 is distant 2,012.35 light years from the Sun and it is moving towards the Sun at the speed of 18 kilometers per second.
Spectral properties of HR8327
HR8327 belongs to spectral class O9 and has a luminosity class of I corresponding to a supergiant star.
The red dot in the diagram below shows where HR8327 is situated in the Hertzsprung–Russell diagram.
HR8327 star system properties
HR8327 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 HR8327 double sysyem: