NGC 3766

E491906

NGC 3766 is a young open star cluster notable for its rich population of hot, massive stars and unusual variable stars, located in the southern sky.

Try in SPARQL Jump to: Statements Referenced by

Statements (47)

Predicate Object
instanceOf open star cluster
young star cluster
age about 14 million years
on the order of 10–30 million years
angularSize about 12 arcminutes
apparentMagnitudeV about 5.3
bestSeenIn binoculars
small telescopes
catalog New General Catalogue NERFINISHED
clusterMass several hundred solar masses
clusterType loose open cluster
contains B-type stars
Be stars
early-type main-sequence stars
hot stars
main-sequence stars
massive stars
pre-main-sequence stars
unusual variable stars
variable stars
declination −61° 36′
discoveredBy Nicolas-Louis de Lacaille NERFINISHED
discoveryYear 1752
distanceFromEarth approximately 1,700 parsecs
approximately 5,500 light-years
environment Galactic disk
estimatedStarCount several hundred member stars
evolutionaryStatus young, still forming massive stars
galacticLatitude approximately +3°
galacticLongitude approximately 294°
hasAlternativeName Caldwell 97 NERFINISHED
Melotte 102 NERFINISHED
hasResearchInterest pulsating variable stars
stellar evolution of massive stars
stellar variability
locatedIn Milky Way
locatedInConstellation Centaurus NERFINISHED
locatedInHemisphere southern celestial hemisphere
notableFor rich population of hot, massive stars
unusual class of variable stars with periods between 0.1 and 0.7 days
observedFrom southern sky
rightAscension 11h 36m
stellarPopulation rich in hot, massive stars
variableStarPopulation includes eclipsing binaries
includes slowly pulsating B-type candidates
includes δ Scuti-like candidates
visibility naked-eye object under dark skies

Referenced by (2)

Full triples — surface form annotated when it differs from this entity's canonical label.