Messier 9

M9, or NGC6333, is a globular cluster in the constellation Ophiuchus. This globular appears quite small on the sky, as it is one of the ones nearer to the galactic center, but it shows a strong central concentration. About 26,000 light-years from us, and about 70 light-years across, M9 looks quite oval due to strong absorption by dust in the north-west (upper right). Only a dozen or so variable stars are known in M9, relatively few for a cluster of its size.

This is a bright globular cluster. In a 8-inch at 188X, the cluster starts to resolve around the edges, and a couple of pinpricks are visible across the middle. The stars are difficult to resolve with direct vision, but they really start to pop out with averted vision.
You can find more information about this Messier object by visiting: SEDS - The Messier Catalog.


    M9
    NGC 6333
    Other description: Globular cluster mottled.
    Constellation: Ophiuchus
    Dreyer description: Globular cluster, bright, large, round, extremely compressed middle, well resolved, stars of magnitude 14; = M9.
    Magnitude: 7.9
    RA: 17h 19m 27.7s Dec: -18°31'23"
    RA: 17h 19m 12.0s Dec: -18°31'00" (Epoch 2000)
    Azm: 186°15'12" Alt: +24°58'13"
    Rise: 19:26 Transit: 00:07 Set: 04:51
    Size: 9.3'

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