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Constellation, Cha

Chamaeleon: the Chameleon

Chamaeleon covers 131 square degrees of sky, the 79th largest of the 88. Its brightest star is star HIP 40702. It is best placed in the evening sky in April.

Show Chamaeleon in the live sky

Chamaeleon at a glance

Chamaeleon: facts from the IAU boundaries and star catalogue
FactValue
IAU abbreviationCha
Meaningthe Chameleon
Pronouncedcuh-MEAL-yun, cuh-MEAL-ee-un
Genitive, used in star namesChamaeleontis (for example a Bayer name such as α Chamaeleontis)
Area131 square degrees, number 79 of 88 by size
Stars to magnitude 6 in our catalogue19
Brightest starstar HIP 40702, magnitude 4.1
Best seenEvenings in April, when it is highest at 9 pm
Declination range-83° to -75°
BordersOctans, Musca, Carina, Apus, Mensa, Volans

Where on Earth you can see Chamaeleon

Chamaeleon spans declinations -83° to -75°. Every part of it rises above the horizon at some moment for observers between latitudes 90°S and 7°N. Some of it can be seen from latitudes 90°S to 15°N. South of 15°S none of it ever sets. This is geometry only: it ignores haze, hills and buildings near the horizon.

From six cities

Chamaeleon from six cities. Altitude is how high its middle gets.
CityLatitudeVisibilityMiddle at its highest
Pune18.5°NNever risesbelow the horizon
New York40.7°NNever risesbelow the horizon
London51.5°NNever risesbelow the horizon
Tromsø69.6°NNever risesbelow the horizon
Tokyo35.7°NNever risesbelow the horizon
Sydney33.9°SNever sets44°

Chamaeleon's named stars

None of the stars brighter than magnitude 6 in Chamaeleon has a name approved by the IAU Working Group on Star Names.

How these facts were found

The name, meaning and boundaries are the IAU's. Area, borders and the latitude ranges are computed from those boundaries; the brightest star and the star count come from a magnitude-6 star catalogue; star names are matched to the catalogue by Hipparcos number and checked by position. The month is when Chamaeleon's middle crosses the north-south line of the sky at 9 pm local solar time. See How we know.

Sources