CVn · Canum Venaticorum
Canes Venatici Constellation
IAU constellation mapCVnCanes Venatici (CVn) is one of the 88 constellations recognised by the International Astronomical Union. It covers 465 square degrees of the northern sky in quadrant NQ3. Its brightest star is Cor Caroli. The Latin genitive of the name is Canum Venaticorum, used to form star names within the constellation. The IAU standardised all constellation boundaries in 1930.
Quick facts
- IAU name
- Canes Venatici
- Abbreviation
- CVn
- Latin genitive
- Canum Venaticorum
- Hemisphere
- northern
- Area
- 465 sq deg
- Brightest star
- Cor Caroli
- Quadrant
- NQ3
- Family
- Ursa Major
- Discovery era
- Johannes Hevelius, 1687
Overview
Canes Venatici is one of the 88 constellations formally recognised by the International Astronomical Union (IAU). It occupies 465 square degrees of sky in the northern hemisphere sky, best visible at latitudes between +90 and -60 degrees in June. The constellation belongs to the Ursa Major family of constellations. Its Latin genitive is Canum Venaticorum, the form used when naming stars within the constellation — for example, the brightest star Cor Caroli may appear in catalogues as Alpha Canum Venaticorum or similar. The IAU standardised the boundaries of all 88 constellations in 1930 under the direction of Eugène Delporte, using straight lines of right ascension and declination to eliminate the ambiguities of earlier variable-boundary systems.
Notable stars
The brightest star in Canes Venatici is Cor Caroli. Individual stars within Canes Venatici are conventionally named using Bayer designation — Greek letters followed by the Latin genitive of the constellation name (Canum Venaticorum) — introduced by Johann Bayer in his 1603 star atlas Uranometria. Flamsteed numbers (numeric designators followed by Canes Venatici) were added by John Flamsteed in his 1712 catalogue. Variable stars, double stars, and deep-sky objects within the Canes Venatici boundary are catalogued by the IAU with the abbreviation CVn.
History and catalogue
Canes Venatici was introduced or documented by Johannes Hevelius, 1687. The modern IAU constellation boundaries were formally established in 1930. The designation CVn is the official three-letter IAU abbreviation used in star catalogues, variable star designations, and positional references. The family classification 'Ursa Major' groups this constellation with others sharing a region of sky or a common historical source in astronomical literature.
Sources & further reading (2)
- official-iau — accessed 2026-05-06
- encyclopedia — accessed 2026-05-06
Frequently asked questions
What does the name Canes Venatici mean?
Canes Venatici is the Latin name used by the IAU to designate this constellation. The name comes from classical Latin and Greek astronomical tradition. In star catalogues, stars within Canes Venatici are designated using the genitive form of the name (e.g. Alpha Canes Venatici or similar Latin genitive forms) — a naming convention introduced by Johann Bayer in his 1603 atlas Uranometria and still in use today.
How large is Canes Venatici compared to other constellations?
Canes Venatici covers 465 square degrees of sky. The full sphere of the sky contains 41,253 square degrees, so Canes Venatici occupies about 1.1% of the total sky. For comparison, the largest constellation is Hydra at 1303 square degrees; the smallest is Crux at 68 square degrees.
When and where is Canes Venatici visible?
Canes Venatici is primarily a northern hemisphere constellation, best seen from mid-northern latitudes. Southern hemisphere observers may see it low on the horizon depending on their latitude. The brightest star, Cor Caroli, serves as the main visual anchor for locating the constellation. As with all constellations, the best viewing conditions are a dark sky away from artificial light pollution, with the constellation high enough above the horizon to minimise atmospheric absorption.
