Celestial hemisphere:  Southern  ·  Constellation: Sagittarius (Sgr)  ·  Contains:  M 22  ·  NGC 6656
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M22, George Simon
M22
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M22

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M22, George Simon
M22
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M22

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Description

Because, at first glance, most globular clusters appear almost identical to every other globular cluster that one has ever observed, globs tend to be underappreciated and less frequently imaged by astrophotographers. However, more careful consideration reveals that most globs can, in fact be distinguished from each other. Such is certainly the case for M22, the Sagittarius Cluster. To begin with, because it lies between us and a portion of the Milky Way's central galactic bulge, it is not set against the sparse star field that typically surrounds most other globular clusters. Instead, it is set against a dense and colorful star field. Next, it is considerably less spherical than the "average" glob; it is, in fact, elliptical, with its major axis running from the upper left to the lower right in my image. M22 is also distinguished by the fact that it is one of only four Milky Way globs known to contain a planetary nebula. It has also been found to contain two stellar-mass black holes. The discovery of these black holes has led astronomers to conclude that stellar-mass black holes are not ejected as efficiently from globs as previously thought. As a result, M22 is conjectured to contain anywhere from 5 to 100 such black holes lurking within its 70-light-year diameter. Finally, Hubble has revealed the presence of 6 planet-sized objects within M22, not gravitationally bound to any particular star. These might be rogue planets and/or brown dwarfs. An appreciation of all these distinguishing characteristics certainly leads to the conclusion that, first appearances notwithstanding, the Sagittarius Cluster is not just another big ball of stars!

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M22, George Simon

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