HR5110 is a variable sub-giant star in the constellation of Canes Venatici.
HR5110 visual magnitude is 4.98. Because of its moderate brightness, HR5110 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 HR5110:
Celestial coordinates and finder chart of HR5110
HR5110 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 HR5110 are provided in the following table:
The simplified sky map below shows the position of HR5110 in the sky:
Visibility of HR5110 from your location
Digitized Sky Survey image of HR5110
The image below is a photograph of HR5110 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 HR5110 is 0.086 arcsec per year in Right Ascension and -0.009 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR5110 from the Sun and relative movement
HR5110 is distant 145.15 light years from the Sun and it is moving far from the Sun at the speed of 7 kilometers per second.
Spectral properties of HR5110
HR5110 belongs to spectral class F2 and has a luminosity class of IV corresponding to a sub-giant star.
The red dot in the diagram below shows where HR5110 is situated in the Hertzsprung–Russell diagram.