Canes Venatici
Constellation in the northern celestial hemisphere From Wikipedia, the free encyclopedia
Constellation in the northern celestial hemisphere From Wikipedia, the free encyclopedia
Canes Venatici (/ˈkeɪniːz vɪˈnætɪsaɪ/) is one of the 88 constellations designated by the International Astronomical Union (IAU). It is a small northern constellation that was created by Johannes Hevelius in the 17th century. Its name is Latin for 'hunting dogs', and the constellation is often depicted in illustrations as representing the dogs of Boötes the Herdsman, a neighboring constellation.
| Constellation | |
| |
| Abbreviation | CVn |
|---|---|
| Genitive | Canum Venaticorum |
| Pronunciation | /ˈkeɪniːz vɪˈnætɪsaɪ/ KAY-neez vih-NAT-ih-seye,[1] genitive /ˈkeɪnəm vɪnætɪˈkɒrəm/ |
| Symbolism | the Hunting Dogs |
| Right ascension | 12h 06.2m to 14h 07.3m |
| Declination | +27.84° to +52.36°[2] |
| Area | 465 sq. deg. (38th) |
| Main stars | 2 |
| Bayer/Flamsteed stars | 21 |
| Stars with planets | 4 |
| Stars brighter than 3.00m | 1 |
| Stars within 10.00 pc (32.62 ly) | 2 |
| Brightest star | Cor Caroli (Asterion) (α CVn) (2.90m) |
| Messier objects | 5 |
| Meteor showers | Canes Venaticids |
| Bordering constellations | |
| Visible at latitudes between +90° and −40°. Best visible at 21:00 (9 p.m.) during the month of May. | |
Cor Caroli is the constellation's brightest star, with an apparent magnitude of 2.9. La Superba (Y CVn) is one of the reddest naked-eye stars and one of the brightest carbon stars. The Whirlpool Galaxy is a spiral galaxy tilted face-on to observers on Earth, and was the first galaxy whose spiral nature was discerned. In addition, quasar Ton 618 is one of the most massive black holes with the mass of 66 billion solar masses.
The stars of Canes Venatici are not bright. In classical times, they were listed by Ptolemy as unfigured stars below the constellation Ursa Major in his star catalogue.
In medieval times, the identification of these stars with the dogs of Boötes arose through a mistranslation: some of Boötes's stars were traditionally described as representing the club (Greek: κολλοροβος, kollorobos) of Boötes. When the Greek astronomer Ptolemy's Almagest was translated from Greek to Arabic, the translator Hunayn ibn Ishaq did not know the Greek word and rendered it as a similar-sounding compound Arabic word for a kind of weapon, writing العصا ذات الكُلاب al-'aşā dhāt al-kullāb, which means 'the staff having a hook'.
When the Arabic text was later translated into Latin, the translator, Gerard of Cremona, mistook كُلاب kullāb ('hook') for كِلاب kilāb ('dogs'). Both written words look the same in Arabic text without diacritics, leading Gerard to write it as Hastile habens canes ('spearshaft-having dogs').[3] In 1533, the German astronomer Peter Apian depicted Boötes as having two dogs with him.[4]
These spurious dogs floated about the astronomical literature until Hevelius decided to make them a separate constellation in 1687.[5] Hevelius chose the name Asterion[lower-alpha 1] for the northern dog and Chara[lower-alpha 2] for the southern dog, as Canes Venatici, 'the hunting dogs', in his star atlas.[7]
In his star catalogue, the Czech astronomer Antonín Bečvář assigned the names Asterion to β CVn and Chara to α CVn.[8]
Although the International Astronomical Union dropped several constellations in 1930 that were medieval and Renaissance innovations, Canes Venatici survived to become one of the 88 IAU designated constellations.[9]
Canes Venatici is bordered by Ursa Major to the north and west, Coma Berenices to the south, and Boötes to the east. The three-letter abbreviation for the constellation, as adopted by the International Astronomical Union in 1922, is "CVn".[10] The official constellation boundaries, as set by Belgian astronomer Eugène Delporte in 1930,[9] are defined by a polygon of 14 sides.
In the equatorial coordinate system, the right ascension coordinates of these borders lie between 12h 06.2m and 14h 07.3m , while the declination coordinates are between +27.84° and +52.36°.[2] Covering 465 square degrees, it ranks 38th of the 88 constellations in size.
Canes Venatici contains no very bright stars. The Bayer designation stars, Alpha and Beta Canum Venaticorum are only of third and fourth magnitude respectively. Flamsteed catalogued 25 stars in the constellation, labelling them 1 to 25 Canum Venaticorum (CVn); however, 1 CVn turned out to be in Ursa Major, 13 CVn was in Coma Berenices, and 22 CVn did not exist.[11]
The Giant Void, an extremely large void (part of the universe containing very few galaxies), is within the vicinity of this constellation. It is regarded to be the second largest void ever discovered, slightly larger than the Eridanus Supervoid and smaller than the proposed KBC Void and 1,200 times the volume of expected typical voids. It was discovered in 1988 in a deep-sky survey. Its centre is approximately 1.5 billion light-years away.[22]
Canes Venatici contains five Messier objects, including four galaxies. One of the more significant galaxies in Canes Venatici is the Whirlpool Galaxy (M51, NGC 5194) and NGC 5195, a small barred spiral galaxy that is seen face-on. This was the first galaxy recognised as having a spiral structure, this structure being first observed by Lord Rosse in 1845.[12] It is a face-on spiral galaxy 37 million light-years from Earth. Widely considered to be one of the most beautiful galaxies visible, M51 has many star-forming regions and nebulae in its arms, coloring them pink and blue in contrast to the older yellow core. M 51 has a smaller companion, NGC 5195, that has very few star-forming regions and thus appears yellow. It is passing behind M 51 and may be the cause of the larger galaxy's prodigious star formation.[23]
Other notable spiral galaxies in Canes Venatici are the Sunflower Galaxy (M63, NGC 5055), M94 (NGC 4736), and M106 (NGC 4258).
Ton 618 is a hyperluminous quasar and blazar in this constellation, near its border with the neighboring Coma Berenices. It possesses a black hole with a mass 66 billion times that of the Sun, making it one of the most massive black holes ever measured.[28] There is also a Lyman-alpha blob.[29]
