Celestial hemisphere:  Southern  ·  Constellation: Ophiuchus (Oph)  ·  Contains:  HD149123  ·  M 107  ·  NGC 6171
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M107 Globular Cluster, Chris Ashford
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M107 Globular Cluster

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M107 Globular Cluster, Chris Ashford
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M107 Globular Cluster

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Description

Half the size of M10, which I imaged on the same night. M107 is only ~10 arcminutes in diamter.

Wikipedia: Messier 107 or M107, also known as NGC 6171 or the Crucifix Cluster, is a very loose globular cluster in a very mildly southern part of the sky close to the equator in Ophiuchus, and is the last such object in the Messier Catalogue.

It was discovered by Pierre Méchain in April 1782, then independently by William Herschel in 1793. Herschel's son, John, in his 1864 General Catalogue, described it as a "globular cluster of stars, large, very rich, very much compressed, round, well resolved, clearly consisting of stars".[5] It was not until 1947 that Helen Sawyer Hogg added it and three other objects found by Méchain to the modern Catalogue, the latter having contributed several of the suggested observation objects which Messier had verified and added.[9] The cluster is to be found 2.5° south and slightly west of the star Zeta Ophiuchi.[5]

M107 is close to the galactic plane and about 20,900 light-years from Earth[3] and 9,800 ly (3,000 pc) from the Galactic Center.[10] Its orbit is partly as far out as the galactic halo, as is between 9,200–12,400 ly (2,820–3,790 pc) from the Galactic Center, the lower figure, the "perigalactic distance" sees it enter and leave the galactic bar.[11]

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M107 Globular Cluster, Chris Ashford