HR5214 is a sub-giant star in the constellation of Canes Venatici.
HR5214 visual magnitude is 6.65. Because of its reltive faintness, HR5214 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 HR5214:
Celestial coordinates and finder chart of HR5214
HR5214 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 HR5214 are provided in the following table:
The simplified sky map below shows the position of HR5214 in the sky:
Visibility of HR5214 from your location
Digitized Sky Survey image of HR5214
The image below is a photograph of HR5214 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 HR5214 is 0.031 arcsec per year in Right Ascension and -0.01 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR5214 from the Sun and relative movement
HR5214 is distant 290.04 light years from the Sun and it is moving towards the Sun at the speed of 12 kilometers per second.
Spectral properties of HR5214
HR5214 belongs to spectral class A5 and has a luminosity class of IV corresponding to a sub-giant star.
The red dot in the diagram below shows where HR5214 is situated in the Hertzsprung–Russell diagram.