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Clusters/Globulars

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M 92, Herkules
18.08.2008, 4" TMB
SXV-H9, L:R:G:B:12:15:15:15, binning 1x1
M 92, Herkules 18.08.2008, 4" TMB SXV-H9, L:R:G:B:12:15:15:15, binning 1x1
M56, Lyra
09.2008 SXV-H9 older image
M56, Lyra 09.2008 SXV-H9 older image
NGC6791, Lyra
09.2008, older SXV-H9 image
NGC6791, Lyra 09.2008, older SXV-H9 image
M3, Canes Venatici
08.2009 older SXV-H9 image
M3, Canes Venatici 08.2009 older SXV-H9 image
M38
03.2010 SXV-H9 older image
M38 03.2010 SXV-H9 older image
M13, Herkules,
24.10.2010, 4" TMB
SV-H9
M13, Herkules, 24.10.2010, 4" TMB SV-H9
M 45
M45, Pleiaden 5.3.2013, 4" TMB f/6.3 | 9x 10 min. | ISO 1600
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Nature and Astrophotography


Mike Androsch



New - October 2026


NGC 6992 in Cygnus, 5.-7. Oct. 2026

Nikon D7500a, 600mm f/4

ISO 1600, 66 x 5 min. (5.5 h)


 After many months of bird photography, I mounted my trusty 600mm f/4 lens on my telescope mount again and was happy to get everything working again.


In the constellation of Cygnus the Swan, there are remnants of a supernova explosion. The source of the supernova was a star 20 times more massive than our sun, which exploded between 10,000 and 20,000 years ago. At the time of the explosion, the supernova would have appeared brighter than Venus in the sky, and was visible in the daytime. The remnants have since expanded to cover an area of the sky roughly 3 degrees in diameter, 36 times the area of the full Moon. The brighter parts of the Cygnus Loop as it is also called, have their own names and this part is designated NGC 6992 (info with the help of wikipedia). It just fit on my chip.
Because there are so many milky way stars in the area, I am also showing an image where my software removed them, so you can see the nebula more clearly. The shock waves are still pushing out hydrogen (red) and oxygen (blue) from the original star.

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