25 Canum Venaticorum

25 Canum Venaticorum is a multiple giant star in the constellation of Canes Venatici.

25 Canum Venaticorum visual magnitude is 4.82. Because of its moderate brightness, 25 Canum Venaticorum should be easily visible from locations with dark skies, while it can be barely visible, or not visible at all, from skies affected by light pollution.

The proper motion of 25 Canum Venaticorum is -0.099 arcsec per year in Right Ascension and 0.027 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.

Key facts about 25 Canum Venaticorum

Celestial coordinates and finder chart of 25 Canum Venaticorum

25 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 25 Canum Venaticorum are provided in the following table:

The simplified sky map below shows the position of 25 Canum Venaticorum in the sky:

Visibility of 25 Canum Venaticorum from your location

Today's 25 Canum Venaticorum rise, transit and set times from Greenwich, United Kingdom are the following (all times relative to the local timezone Europe/London):

Distance of 25 Canum Venaticorum from the Sun and relative movement

25 Canum Venaticorum is distant 191.65 light years from the Sun and it is moving towards the Sun at the speed of 6 kilometers per second.

Spectral properties of 25 Canum Venaticorum

25 Canum Venaticorum belongs to spectral class A7 and has a luminosity class of III corresponding to a giant star.

The red dot in the diagram below shows where 25 Canum Venaticorum is situated in the Hertzsprung–Russell diagram.

25 Canum Venaticorum star system properties

25 Canum Venaticorum is a visual double star which can be observed with the help of medium or large telescopes. The table below shows key information about the 25 Canum Venaticorum double sysyem:

Alternative designations of 25 Canum Venaticorum