NGC 6342
{{Short description|Globular cluster in the constellation Ophiuchus}}
{{Infobox globular cluster
| name = NGC 6342
| image = 250px
| caption = NGC 6342 as seen through the Hubble Space Telescope
| epoch = J2000
| pronounce =
| constellation = Ophiuchus
| z =
| h_radial_v = {{val|+115.7|1.4|u=km/s}}
| gal_v =
| dist_pc =
| dist_ly =
| group_cluster =
| mass =
| mass_light_ratio =
| size =
| stars =
| size_v = 4.40{{prime}}
| notes =
| names = GCL 61 and ESO 587-SC6
| references = NASA/IPAC extragalactic datatbase, http://spider.seds.org/
}}
NGC 6342 is a globular cluster located in the constellation Ophiuchus. Its Shapley–Sawyer Concentration Class is IV,{{cite web|title=Revised NGC Data for NGC 6342|url=http://spider.seds.org/ngc/revngcic.cgi?NGC6342|website=Seds|access-date=14 October 2015}} and it was discovered by the German-born British astronomer William Herschel on 28 May 1786.{{cite web|title=NGC 6342 (= GCL 61)|url=http://cseligman.com/text/atlas/ngc63.htm#6342|website=cseligman|access-date=14 October 2015}} It is at a distance of 28,000 light years away from Earth.{{cite web|title=NGC 6342|url=http://spider.seds.org/spider/MWGC/n6342.html|website=Seds|access-date=14 October 2015}}{{cite web|title=The globular cluster NGC 6342|url=https://in-the-sky.org/data/object.php?id=5097|website=In-the-sky|access-date=14 October 2015}}
NGC 6342 is classified as metal-rich, yet has only one generation of stars.
See also
References
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External links
- {{commons category-inline}}
{{Ngc65}}
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