HR5077 is a giant star in the constellation of Canes Venatici.
HR5077 visual magnitude is 6.47. Because of its reltive faintness, HR5077 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 HR5077:
Celestial coordinates and finder chart of HR5077
HR5077 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 HR5077 are provided in the following table:
The simplified sky map below shows the position of HR5077 in the sky:
Visibility of HR5077 from your location
HR5077 is circumpolar and transits at 18:29 UTC (altitude: 79.2°)
Digitized Sky Survey image of HR5077
The image below is a photograph of HR5077 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 HR5077 is 0.009 arcsec per year in Right Ascension and -0.056 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR5077 from the Sun and relative movement
HR5077 is distant 431.79 light years from the Sun and it is moving towards the Sun at the speed of 58 kilometers per second.
Spectral properties of HR5077
HR5077 belongs to spectral class G8 and has a luminosity class of III corresponding to a giant star.
The red dot in the diagram below shows where HR5077 is situated in the Hertzsprung–Russell diagram.