HR5245 is a sub-giant star in the constellation of Canes Venatici.
HR5245 visual magnitude is 6.32. Because of its reltive faintness, HR5245 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 HR5245:
Celestial coordinates and finder chart of HR5245
HR5245 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 HR5245 are provided in the following table:
The simplified sky map below shows the position of HR5245 in the sky:
Visibility of HR5245 from your location
Digitized Sky Survey image of HR5245
The image below is a photograph of HR5245 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 HR5245 is -0.118 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.
Distance of HR5245 from the Sun and relative movement
HR5245 is distant 236.06 light years from the Sun and it is moving towards the Sun at the speed of 22 kilometers per second.
Spectral properties of HR5245
HR5245 belongs to spectral class F4 and has a luminosity class of IV corresponding to a sub-giant star.
The red dot in the diagram below shows where HR5245 is situated in the Hertzsprung–Russell diagram.