Introduction | Map | Find/Identify | Sketch | My Best Own Photos | My Own Observations | References || Appendix: My Own Photos
On this page I collect my observations of the globular star cluster M 13 (NGC 6205) in the constellation Hercules. In the neighborhood there is the spiral galaxy NGC 6207.
The globular star cluster M 13 in the Hercules constellation is probably the largest globular cluster in the northern sky. It is located on the right edge of the Keystone asterism, which is the most prominent part of the constellation Hercules and forms a trapezoid. M 13 is not quite round and, depending on the author, 8 'or 15' in size. I was able to see the bright nucleus well, but I was not able to resolve single stars - until August 23, 2019, on which I suceeded using averted vision (and maybe also with direct vision...) for the first time.
Helpful for the visual search are the two stars which form an obtuse triangle with M 13 (see further down). In the neighborhood there is the spiral galaxy NGC 6207.
M 13 (NGC 6205) | NGC 6207 | |
Size: 8' / 15' (Stoyan/Karkoschka) Distance: 24,000 light years (Stoyan) Rating: **** (Stoyan) |
Size: 3.5' x 1.2' (Wikipedia) Distance: 45 mio. light years (Wikipedia) Rating: --- |
M 13 is located at the right edge of the Keystone asterism (1/3 from the top) (Image Courtesy of SkySafari Astronomy, www.simulationcurriculum.com)
Find: The globular star cluster M 13 in the constellation Hercules is located at the right edge of the Keystone asterism (1/3 from the top) and therefore easy to find once you have found the Keystone trapezoid.
Identify: When you look more closely at the region of M 13, you will find two stars to the left of M 13; these form, together with M 13, a triangle, which can be seen well in binoculars or at low magnifications and serves for safe identification (Image Courtesy of SkySafari Astronomy, www.simulationcurriculum.com). Here is a detail view of the triangle (created with Stellarium):
Overall, this cluster is an easy-to-find object, even with binoculars, at least once you have found the Keystone asterism. Helpful are also the two stars with which M 13 forms an obtuse triangle.
The sketch by Michael Vlasov (DeepSkyWatch.com) provides a rough impression of what I observed in Summer/Autumn 2016 (my impression was much fainter and smaller than the sketch):
Sketch of the M 13 globular star cluster by Michael Vlasov (Copyright © Michael Vlasov 2016) - presented with the author's permission
M 13 - Aug 22, 2022 |
M 13 - Aug 21, 2023 | M 13 - Sep 6, 2023, 5 min | ||
M 13 - Aug 22, 2022, photo on top processed |
M 13 - Aug 21, 2023, photo on top processed |
M 13 - Sep 6, 2023, photo on top processed |
M 13, Aug 12, 2022 - original (30 frames = 300 seconds) |
M 13, Aug 20, 2022 - original (89 frames = 890 seconds) |
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M 13, Aug 25, 2022 - original (90 frames = 900 seconds) |
M 13, Aug 28, 2022 - original (30 frames = 300 seconds) |
M 13, Jun 4, 2024 - 2000p (90 frames = 900s) |
M 13, Jun 4, 2024 - 2000p (90 frames = 900s), processed |
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M 13 & NGC 6207 (left), Jun 4, 2024 - 1800p (90 frames = 900s), 1:1 section, processed |
Evaluation with nova.astrometry.net |
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M 13 & NGC 6207 (left), Jun 4, 2024 - 2000p (90 frames = 900s), processed (Siril) |
M 13, Jun 4, 2024 - 1800p (90 frames = 900s), 1:1 section, processed (Siril) |
M 13, Jul 29, 2022 - original (20 frames = 200 seconds) |
M 13, Jul 30,2022 - original (89 frames = 890 seconds) |
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M 13, Jul 31, 2022 - original (60 frames = 600 seconds) |
M 13, Aug 6, 2022 - original (40 frames = 400 seconds) |
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M 13, Aug 12, 2022 - original (30 frames = 300 seconds) |
M 13, Aug 20, 2022 - original (89 frames = 890 seconds) |
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M 13, Aug 25, 2022 - original (90 frames = 900 seconds) |
M 13, Aug 28, 2022 - original (30 frames = 300 seconds) |
M 13, Jun 4, 2024 - 2000p (90 frames = 900s) |
M 13, Jun 4, 2024 - 2000p (90 frames = 900s), processed |
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M 13 & NGC 6207 (left), Jun 4, 2024 - 1800p (90 frames = 900s), 1:1 section, processed |
Evaluation with nova.astrometry.net |
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M 13 & NGC 6207 (left), Jun 4, 2024 - 2000p (90 frames = 900s), processed (Siril) |
M 13, Jun 4, 2024 - 1800p (90 frames = 900s), 1:1 section, processed (Siril) |