HR9005 is a sub-giant star in the constellation of Cepheus.
HR9005 visual magnitude is 5.95. Because of its reltive faintness, HR9005 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 HR9005:
Celestial coordinates and finder chart of HR9005
HR9005 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 HR9005 are provided in the following table:
The simplified sky map below shows the position of HR9005 in the sky:
Visibility of HR9005 from your location
HR9005 is circumpolar and transits at 14:40 UTC (altitude: 74.7°)
Digitized Sky Survey image of HR9005
The image below is a photograph of HR9005 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 HR9005 is 0.004 arcsec per year in Right Ascension and 0.001 arcsec per year in Declination and the associated displacement for the next 100000 years is represented with the red arrow.
Distance of HR9005 from the Sun and relative movement
HR9005 is distant 1,734.04 light years from the Sun and it is moving towards the Sun at the speed of 14 kilometers per second.
Spectral properties of HR9005
HR9005 belongs to spectral class B2 and has a luminosity class of IV corresponding to a sub-giant star.
The red dot in the diagram below shows where HR9005 is situated in the Hertzsprung–Russell diagram.