Beehive Cluster

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This article is about the Beehive Cluster. For other uses, see Beehive.

**Beehive Cluster**
Observation data (Epoch J2000.0)
Globular cluster	List of globular clusters

Class	II,2,m
Constellation	Cancer
Right ascension	08^h 40.1^m
Declination	19° 51′
Distance	0.577 kly (177 Pc)
Apparent magnitude (V)	3.7
Apparent dimensions (V)	95′
Physical characteristics
Mass	( M_☉)
Radius	16 light years
V_HB
Estimated age	730 million years
Notable features
Other designations	M44, Praesepe, NGC 2632

The Beehive Cluster (also known as Praesepe (Latin for "manger"), M44 or NGC 2632) is an open cluster in the constellation Cancer. It looks like a nebulous object to the naked eye under dark skies, and thus has been known since ancient times--Ptolemy called it "The nebulous mass in the breast" of Cancer. It is also among the first objects Galileo studied with his telescope.

The 730-million-year old cluster is 577 light years away; its age and proper motion coincide with the Hyades open cluster, suggesting they were created in the same diffuse nebula. Both contain red giants and white dwarfs, but the brightest stars are class A, F, and G stars. It contains at least 200 stars, and perhaps as many as 350.

The Beehive is most easily observed in the spring, when Cancer is high in the sky. At 95 arc minutes across, it fits well in the field of view of binoculars or a telescope of low power.

1 History
2 Composition
3 References
4 External links

[edit] History

Ancient Greeks and Romans saw this nebulous object as a manger with two donkeys, the stars Asellus Borealis and Asellus Australis, eating from it, specifically, the donkeys that Dionysos and Silenus rode into battle against the Titans.<ref>M44, Students for the Exploration and Development of Space, February 6, 2005.</ref>

Galileo was the first to observe the Beehive in a telescope, in 1609, and was able to resolve it into 40 stars. Charles Messier added it to his famous catalog in 1769 after precisely measuring its position in the sky. Along with the Orion Nebula and the Pleiades cluster, Messier's inclusion of the beehive has been noted as curious, as most of Messier's objects were much fainter and more easily confused with comets. One possibility is that Messier simply wanted to have a larger catalogue than his scientific rival Lacaille, whose 1755 catalogue contained 42 objects, and so he added some bright, well-known objects to boost his list<ref>Frommert, Hartmut (1998). "Messier Questions & Answers". Retrieved March 1, 2005.</ref>

[edit] Composition

The cluster is about 16 light years in diameter and contains at least 200 stars confirmed to be bound to the cluster, out of 350 total in the vicinity. It has a visual brightness of magnitude 3.7. Its brightest stars are blue-white and of magnitude 6 to 6.5. The Beehive is one of the older and larger open clusters known.

42 Cancri is a member of this cluster.