Puppis Clusters

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Puppis Clusters

Early 1771 was a busy time for Charles Messier. The French astronomer was most interested in discovering comets. To make the process faster, he compiled a list of objects that resembled comets: galaxies, gas clouds, and star clusters. He could ignore the objects on the list, reducing the number of false alarms.

And 250 years ago, he recorded four of them. Two of them are clusters in the constellation Puppis: Messier 46 and 47. They stand side by side — so close together that they’re in the same field of view through binoculars.

M47 is the brighter of the two. It’s about 1600 light-years away, and consists of several hundred stars. The cluster is still pretty young, so some of its more massive stars haven’t yet had time to burn out. They’re especially bright, and they shine blue-white, so they overpower most of the rest of the cluster. A couple of massive stars are at the ends of their normal lifetimes. They’ve gotten bigger and cooler, so they look red or orange.

M46 is fainter than M47 in part because it’s about three times as far as M47. But it’s also because the cluster is about three times as old. Its heaviest and most vigorous stars have already expired, leaving it with fewer standouts to draw attention.

The clusters are in the south as night falls. They’re not far to the upper left of Sirius, the brightest star in the night sky. Messier 46 stands close to the left of its brighter neighbor.

Script by Damond Benningfield

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