Canis Major

1790 OBJECTS
Canis Major · 28° of sky top to bottom · stars to magnitude 6.5 · figure by the IAU and Sky & Telescope

Canis Major holds Sirius, the brightest star in the night sky — bright chiefly because it is close, at 8.6 light years, which puts it among the nearest handful of star systems to the Sun. Sirius has a white dwarf companion about the size of the Earth and about the mass of the Sun, predicted from a wobble in its motion and then seen in 1862. The constellation sits in the winter Milky Way and carries the bright open cluster M 41 a few degrees south of Sirius.

Canis Major holds 1790 catalogued objects: 1386 stars, 341 galaxies, 33 exoplanets, 14 star clusters, 10 neutron stars, 4 nebulae, 2 unclassified.

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THE FAMOUS ONES

] 1 ENTRIES
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BRIGHTEST OBJECTS

] 12 SHOWN
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COMMON QUESTIONS

] 8 ANSWERED
Where in the sky is Canis Major?
Its boundary is centred near right ascension 6h 41m, declination −23.4°. It stands at its highest around midnight in late December, which puts it in the evening sky for the two months after that and behind the Sun half a year later.
Can I see it from where I live?
Every part of Canis Major clears the horizon from latitudes between the south pole and 50° N. Outside that band some or all of the region never rises at all, whatever the time of year — a constellation is fixed on the sky, and it is your latitude that decides how much of the sky you get.
What is the brightest thing in it?
The brightest catalogued object in Canis Major is Sirius, at apparent magnitude −1.44 (V). That is apparent brightness — how it looks from Earth — so it mixes how much light a thing gives off with how far away it is, and the brightest object in a region is rarely the most interesting one.
How are the stars in it named?
The brightest carry Greek letters, assigned roughly in order of brightness — by Johann Bayer in 1603, and for the deep southern constellations by Nicolas-Louis de Lacaille in the 1750s — followed by the Latin genitive of the constellation's name. Fainter naked-eye stars north of about −30° take a number from John Flamsteed's catalogue, which never covered the far south, and fainter still a designation from whichever survey recorded them.
What exactly are the boundaries?
Lines of constant right ascension and declination, drawn by Eugène Delporte for the IAU in 1930 and referred to the sky as it stood in 1875. Precession has tilted the sky against them since, which is why the boundaries on a modern chart are very slightly askew.
Are the stars in Canis Major actually near each other?
Almost never. The stars in a constellation lie at wildly different distances and are not related to one another in any way — the pattern is a line of sight from one particular planet. Two stars that look adjacent can be a hundred times further apart than either is from the Sun.
What is the difference between a constellation and an asterism?
A constellation is one of the 88 regions the IAU recognises, with a fixed boundary and an official name. An asterism is any memorable pattern that is not one — the Plough inside Ursa Major, the Summer Triangle drawn across three constellations, the Great Square shared between two.
Why are the names in Latin?
Because the list was assembled in Latin. Fifty of the 88 descend from Ptolemy's second-century catalogue of forty-eight — his ship Argo was later cut into three — and the rest were coined between the sixteenth and eighteenth centuries to fill the southern sky and the gaps. The genitive form is what star names use: Alpha Orionis means the alpha star of Orion.