M46
Messier 46 or M46, also known as NGC 2437, is an open cluster of stars in the constellation of Puppis. It was discovered by Charles Messier in 1771. Dreyer described it as "very bright, very rich, very large." M46 is about 4,920 light-years away. There are an estimated 500 stars in the cluster with a combined mass of 453 M☉, and it is thought to be some 251.2 million years old.
The cluster has a tidal radius of 37.8 ± 4.6 ly (11.6 ± 1.4 pc) and a core radius of 8.5 ± 1.3 ly (2.6 ± 0.4 pc). It has a greater spatial extend in the infrared than in visible light, suggesting that the cluster is undergoing some mass segregation with the fainter (redder) stars migrating to a coma region. The fainter stars that extend out to the south and west may form a tidal tail due to a past interaction.
The planetary nebula NGC 2438 appears to lie within the cluster near its northern edge (the faint smudge at the top center of the image), but it is most likely unrelated since it does not share the cluster's radial velocity. It is an example of a superimposed pair possibly similar to that of NGC 2818. On the other hand, the illuminating star of the bipolar Calabash Nebula shares the radial velocity and proper motion of Messier 46, and is at the same distance, so is a bona fide member of the open cluster.
M46 is located close by to another open cluster, Messier 47. M46 is about a degree east of M47 in the sky, so the two fit well in a binocular or wide-angle telescope field.
