10 Canum Venaticorum

10 Canum Venaticorum is a hypergiant star in the constellation of Canes Venatici.

10 Canum Venaticorum visual magnitude is 5.95. Because of its reltive faintness, 10 Canum Venaticorum 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 10 Canum Venaticorum:

Celestial coordinates and finder chart of 10 Canum Venaticorum

10 Canum Venaticorum 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 10 Canum Venaticorum are provided in the following table:

The simplified sky map below shows the position of 10 Canum Venaticorum in the sky:

Visibility of 10 Canum Venaticorum from your location

10 Canum Venaticorum is circumpolar and transits at 19:53 UTC (altitude: 77.8°)

Digitized Sky Survey image of 10 Canum Venaticorum

The image below is a photograph of 10 Canum Venaticorum 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 10 Canum Venaticorum is -0.355 arcsec per year in Right Ascension and 0.139 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.

Distance of 10 Canum Venaticorum from the Sun and relative movement

10 Canum Venaticorum is distant 56.63 light years from the Sun and it is moving far from the Sun at the speed of 81 kilometers per second.

Spectral properties of 10 Canum Venaticorum

10 Canum Venaticorum belongs to spectral class G0 and has a luminosity class of V corresponding to a hypergiant star.

The red dot in the diagram below shows where 10 Canum Venaticorum is situated in the Hertzsprung–Russell diagram.

Alternative designations of 10 Canum Venaticorum