M92, A Globular Cluster, - this image cropped and reduced from the original photo, Click on photo above for a full resolution image.
Messier object #92 (M92) is considered one of the best of the Globular Cluster types. Personally, from a visual standpoint I find it to be a bit of a let down, especially compared to it's better known and nearby neighbor to the SW,  M13. But M92 is one of the brighter objects, just beyond unaided eye visibility, but easily spotted with 7x35 binoculars. M92 does have some impressive statistics. There are at least 330,000 member stars, many of which are individually resolvable with moderate amateur telescopes, (as you can see in this photo), even though it is over 27,000 light years away, which for comparison is beyond the center of our Milky Way. It is currently coming toward us at over 70 miles per second but on an independent circular orbit around the M.W.'s core, not in the same plane as our sun or the rest of the galaxy.  It is really old, older than most of its kin, and maybe older than the M.W itself. It probably had largely settled into its present shape and size even before the M.W. was well organized, and is a gravitationally captured, independent object. It's 110 light years in diameter, which is why, even at that distance, it is relatively visible and bright.

You can find it to the west of the summer Milky Way, above the left shoulder of Hercules.

11" Celestron HDEdge, F10, moddifiied Schmidt Cassegrain Telescope, Canon Ra camera, placed at the scope's prime focus
8 photos aligned and averaged together, then brightness, color, and contrast enhanced.
Each photo, 25 seconds exposure at ISO 3200