HR5219 is a variable giant star in the constellation of Canes Venatici.
HR5219 visual magnitude is 4.74. Because of its moderate brightness, HR5219 should be easily visible from locations with dark skyes, while it can be barely visible, or not visible at all, from skyes affected by light pollution.
The table below summarizes the key facts about HR5219:
Celestial coordinates and finder chart of HR5219
HR5219 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 HR5219 are provided in the following table:
The simplified sky map below shows the position of HR5219 in the sky:
Visibility of HR5219 from your location
Digitized Sky Survey image of HR5219
The image below is a photograph of HR5219 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 HR5219 is -0.019 arcsec per year in Right Ascension and -0.032 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR5219 from the Sun and relative movement
HR5219 is distant 603.70 light years from the Sun and it is moving towards the Sun at the speed of 44 kilometers per second.
Spectral properties of HR5219
HR5219 belongs to spectral class K5 and has a luminosity class of III corresponding to a giant star.
The red dot in the diagram below shows where HR5219 is situated in the Hertzsprung–Russell diagram.