HR9013 is a main-sequence star in the constellation of Cepheus.
HR9013 visual magnitude is 5.04. Because of its reltive faintness, HR9013 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 HR9013:
Celestial coordinates and finder chart of HR9013
HR9013 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 HR9013 are provided in the following table:
The simplified sky map below shows the position of HR9013 in the sky:
Visibility of HR9013 from your location
HR9013 is circumpolar and transits at 19:08 UTC (altitude: 73.7°)
Digitized Sky Survey image of HR9013
The image below is a photograph of HR9013 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 HR9013 is 0.014 arcsec per year in Right Ascension and -0.001 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR9013 from the Sun and relative movement
HR9013 is distant 297.45 light years from the Sun and it is moving far from the Sun at the speed of 10 kilometers per second.
Spectral properties of HR9013
HR9013 belongs to spectral class A1 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR9013 is situated in the Hertzsprung–Russell diagram.