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2MASS near-infrared telescope survey centred on Beehive
Beehive · Telescope survey view · 2MASS · University of Massachusetts and IPAC/Caltech; funded by NASA and NSF. Colour mosaic and cutout: CDS/Aladin.

Beehive

Star cluster in Cancer · 577 light-years

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TypeStar cluster
ConstellationCancer
Right ascension8h 40m 22s
Declination+19° 40′
Object distance577 light-years
Apparent magnitude3.1
Apparent size108.6′ (arc-minutes)
Approx. true diameter18.2 light-years across
Also known asM44 · NGC 2632 · Praesepe Cluster
Messier 44, popularly known as the Beehive, is a star cluster (also catalogued as NGC 2632) in Cancer — a gravitationally bound family of stars sharing a common origin. It was recorded by Charles Messier in his famous catalogue of 110 deep-sky objects. It spans roughly 108.6 arc-minutes on the sky. At about magnitude 3.1, it is bright enough to glimpse with the unaided eye under a dark sky.

Although it appears about 108.6′ wide on the sky, its real span is roughly 18.2 light-years — the difference is a measure of how far away it lies.

Observing Beehive

Beehive lies in the constellation Cancer and is best placed in the evening sky around January. Its maximum altitude above the horizon depends on your latitude. Lying near the celestial equator, it can be seen from both hemispheres. At its brightness it can be found with the unaided eye under a dark sky and is easy in binoculars.

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Sources

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