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| | Messier Object 92 |
 | | Globular cluster M92 is one of the original discoveries of Johann Elert Bode, who found it on December 27, 1777. |
 | | Only about 16 variables have been discovered in this globular, 14 of which are of RR Lyrae type, while one of them is one of the very few eclipsing binaries in globular clusters, of W Ursae Majoris type. |
 | | Although Burnham claims it is not well understood why eclipsing binaries are so rare in globulars, it appears to the present author that there may be a simple answer: In these dense stellar agglomerates, close encounters occur frequently, so that binary systems will be disturbed, and on the long term, will be destroyed. |
| www.seds.org /messier/m/m092.html (440 words) |
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