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Canes Venatici (Hunting Dogs)

COSMOS / CONSTELLATIONS / CVN

Canes Venatici (Hunting Dogs)

The Hunting Dogs. IAU abbreviation CVn. One of the seven constellations introduced by Johannes Hevelius and published in his star atlas of 1690.

STAR CHART

Cor CaroliChara24 CVn20 CVnHIP 676655 CVn↑ N ← E
Coloured dots are the stars of Canes Venatici brighter than magnitude 6.5 (size by brightness, colour by temperature); grey dots are stars brighter than 5.5 in neighbouring constellations. North is up, east to the left. Constellation boundaries and traditional stick figures are not drawn.

KEY FACTS

IAU abbreviation
CVn
Latin name / genitive
Canes Venatici / Canum Venaticorum
Position
Right ascension ≈ 13 h 12 m; declination +28° to +52°
Visibility from Türkiye
Visible in full from anywhere in Türkiye. When it crosses the meridian its centre stands about 90° above the horizon from Ankara.
Best time to observe
Best placed at 21:00 Türkiye time around 6 June.
Number of stars
61 stars brighter than magnitude 6.5 in the catalogue; 9 brighter than 5 and 1 brighter than 4.

INTERACTIVE LAB

Where is Canes Venatici tonight?

The lab opens for Ankara on today’s date. Drag the time slider through the night; the “Best night” button jumps to the date when the constellation is highest at 21:00 (around 6 June). Change the city to compare the view from elsewhere in Türkiye and around the world.

MYTH, HISTORY AND OBSERVING

Hevelius introduced this constellation in 1687 as the two hunting dogs held on a leash by Boötes. Its brightest star, Cor Caroli, is named after King Charles I of England. It contains the Whirlpool Galaxy (M51), the first galaxy whose spiral structure was drawn, and the bright globular cluster M3.

BRIGHTEST STARS

StarMagnitudeDistance (light-years)Spectral type
Cor Caroli2.89115A0spe
Chara4.2428G0V
24 CVn4.68180A5V
20 CVn4.72264F3III
5 CVn4.76386G7III
HIP 676654.76601K5III
25 CVn4.82199A7III
HIP 662574.91149F2IV

Magnitude: apparent brightness; the smaller the number, the brighter the star. Distances derive from parallax measurements and are uncertain for distant stars. Source: HYG v4.1 star catalogue (CC BY-SA 4.0).

SOURCES

Position, visibility and best observing time were computed approximately for this page from the catalogue stars (Ankara, 39.9° N). The 88 constellations were adopted by the IAU in 1922; their boundaries were drawn by Eugène Delporte in 1930.

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