In addition to its fine appearance when viewed with binoculars or a small telescope, M46 appears to contain a surprise - a small planetary nebula, NGC 2438, which appears as small colored disk at the cluster's edge. Astronomers consider this to be more appearance than actual association since the nebula appears to be moving at a different speed than the cluster, and since the cluster's member stars are too young to have gone nova (the death throes of older stars, which produces planetary nebulae). It is most likely that the nebula lies in front of M46 and simply appears to be part of it.
The image below is a crop of the preceeding image, showing NGC 2438 near the upper middle of the frame, at the top edge of the cluster's core.
The above images were comprised of five, 300-second subexposures - a total exposure time of 25 minutes.
M44
This a large open cluster in the constellation Cancer, also known as the Praesepe (Latin for Manger) or Beehive Cluster. M44 was first noted by Greek and Roman astronomers; Galileo viewed it with his homemade telescope as early as 1609; more than 150 years later Charles Messier added it to his catalog.
M44 has about a thousand member stars, but its members have dispersed over a fairly large area over the eons. It is about 577 light years away and occupies an area larger than the full moon. The cluster is best viewed with binoculars or a telescope with low magnification and a wide field of view.
M103
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