M41 (NGC 2287)

M41. Image credit: NOAO/AURA/NSF

An open open cluster (Trumpler class I, 3, r) that lies in the constellation Canis Major, about 4° due south of Sirius. M41 is approximately 200 million years old. It contains about 100 stars, including several bright red giants, the brightest of which is of spectral type K3 and mag 6.9, and situated near the cluster's center. The bright star in the southeast corner (lower left) of the accompanying image is a foreground blue giant, not part of the cluster.

M41 was discovered by Giovanni Hodierna before 1654, although it has been suggested (by J. E. Gore) that it was known to Aristotle about 325 BC.

visual magnitude	4.5
angular size	38'
linear diameter	25 light-years
distance	2,300 light-years (700 pc)
position	R.A. 06h 46.0m, Dec. -20° 46'
other designations	C 0644-206, OCl 597.0

Related categories

• NEBULAE AND STAR CLUSTERS
• MESSIER CATALOGUE

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