Messier 92 (M 92)

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 92 (NGC 6341) in the constellation Hercules.

 

Introduction

The globular star cluster M 92 in the Hercules constellation is somewhat smaller (depending on the author, it is 7 'or 8' in size) than its more familiar "brethren" M 13. It is located above the Keystone asterism, the most prominent part of the constellation and more difficult to find than M 13. I was able to clearly see the bright nucleus (M 92 appears somewhat more concentrated at the center than M 13), but not dissolve single stars - until August 23, 2019, on which I suceeded using averted vision (and maybe also with direct vision...) for the first time. In my binoculars, M 92 appears also very small.

M 92 (NGC 6341)
Size: 14' (Wikipedia)
Distance: 25,000 light years (Stoyan)
Rating: *** (Stoyan)

 

Map

The globular star cluster M 92 is located above the Keystone asterism and a little more difficult to find than M 13. First find the Keystone asterism! (Image Courtesy of SkySafari Astronomy, www.simulationcurriculum.com)

 

Find/Identify

Find: The globular star cluster M 92 in the constellation Hercules is located above the Keystone asterism and hard to find for me because there are no stars that can be used for orientation:

I therefore try to start from the two upper Keystone stars and form a kind of triangle with them to find M 92, which is generally quite tedious. Another approach is, to go up again about the height of the keystone trapezoid and then go 1/3 of the upper side to the right.

Find (2):In September 2024, I found somewhat brighter stars in the vicinity of M 92, which helped me to clearly "approach" and identify M 92 with binoculars. While SkySafari does not show any stars in the vicinity of M 92, this is the case with Stellarium. And these actually help to locate M 92, because they match what you see with binoculars. M 92 forms the eastern corner of a triangle (as a somewhat "fuzzy star"), while two stars, one above and one below M 92 to the west of M 92, form the other two corners of the triangle. Other stars further to the west help to identify the triangle as such. The star below the triangle is particularly bright. Here is an image of the position of M 92 created with Stellarium:

Identify: If you found a globular cluster in this way, then M 92 is already identified! (Image Courtesy of SkySafari Astronomy, www.simulationcurriculum.com)

 

Sketch

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 92 globular star cluster by Michael Vlasov (Copyright © Michael Vlasov 2016) - presented with the author's permission

 

My Best Own Photos

eVscope

         

M 92 - May 16, 2020

 

M 92 -May 16, 2020, processed

 

M 92 - May 16, 2020, processed and sharpened

         

M 92 - Jun 11, 2020, Sky somewhat bright

 

M 92 - Jun 11, 2020, processed

 

M 92 - Jun 11, 2020, processed and sharpened

         

M 92 - Aug 25, 2020, manual exposure

 

M 92 - Aug 25, 2020, processed

 

M 92 - Aug 25, 2020, processed and sharpened

         

M 92 - Sep 15, 2020, manual exposure

 

M 92 - Sep 15, 2020, processed

 

M 92 - Sep 15, 2020, processed and sharpened

         

M 92 - Jul 18, 2021

 

M 92 - Jul 18, 2021, processed

 

M 92 - Jul 18, 2021, processed and sharpened

         

M 92 - Aug 20, 2021

 

M 92 - Aug 20, 2021, processed

 

M 92 - Aug 20, 2021, processed and sharpened

eVscope 2

         

M 92 - Aug 21, 2023

 

M 92 - Oct 10, 2023, 5 min

 

M 92 - Dec 18, 2023, 3 min

      

M 92 - Aug 21, 2023, photo on top processed

 

M 92 - Oct 10, 2023, photo on top processed

 

M 92 - Dec 18, 2023, photo on top processed

Vespera

M 92, Jul 29, 2022 - original (29 frames = 290 seconds)

Vespera Pro

    

M 92, Jun 4, 2024 - 2000p (90 frames = 900s)

 

M 92, Jun 4, 2024 - 2000p (92 frames = 900s), processed

 

M 92, Jun 4, 2024 - 1800p (90 Frames = 900s), 1:1 section

 

M 92, Jun 4, 2024 - 1800p (90 Frames = 900s), 1:1 section, processed

 

My Own Observations

Observations Summer to Autumn 2016

Observations May 2017

Observations October 2017

Observations September/October 2018

Observations August 2019

Observations September/October 2019

Observations April to October 2020

Observations July to Oktober 2021

Observations July 2022

Observations August to December 2023

Observations June 2024

 

References

On this Site


Appendix: My Own Photos

ZWO ASI224

         

M 92 - Sep 2, 2021, PS 72/432, stacked from single frames

 

M 92 - Sep 3, 2021, C5, 60frames, 5sec, gain300

 

M 92- Sep 4, 2021, TLAPO1027, 60frames, 5sec, gain300

      

M 92 - Sep 2, 2021, PS 72/432, stacked from single frames, processed

 

M 92 - Sep 3, 2021, C5, 60frames, 5sec, gain300, processed

 

M 92- Sep 4, 2021, TLAPO1027, 60frames, 5sec, gain300, processed

eVscope

         

M 92 - Apr 15, 2020

 

M 92 - Apr 15, 2020, processed

 

M 56 - 92 15, 2020, processed and sharpened

         

M 92 - Apr 15, 2020

 

M 92 - Apr 15, 2020, processed

 

M 92 - Apr 15, 2020, processed and sharpened

         

M 92 - May 16, 2020

 

M 92 - May 16, 2020, processed

 

M 92 - May 16, 2020, processed and sharpened

         

M 92 - May 16, 2020

 

M 92 -May 16, 2020, processed

 

M 92 - May 16, 2020, processed and sharpened

         

M 92 - May 16, 2020

 

M 92 - May 16, 2020, processed

 

M 92 - May 16, 2020, processed and sharpened

         

M 92 - Jun 11, 2020, somewhat bright

 

M 92 - Jun 11, 2020, processed

 

M 92 - Jun 11, 2020, processed and sharpened

         

M 92 - Jul 3, 2020, sky too bright

 

M 92 - Jul 3, 2020, processed

 

M 92 - Jul 3, 2020, processed and sharpened

         

M 92 - Aug 19, 2020, manual exposure

 

M 92 - Aug 19, 2020, processed

 

M 92 - Aug 19, 2020, processed and sharpened

         

M 92 - Aug 19, 2020, manual exposure

 

M 92 - Aug 19, 2020, processed

 

M 92 - Aug 19, 2020, processed and sharpened

         

M 92 - Aug 25, 2020, manual exposure

 

M 92 - Aug 25, 2020, processed

 

M 92 - Aug 25, 2020, processed and sharpened

         

M 92 - Sep 15, 2020, manual exposure

 

M 92 - Sep 15, 2020, processed

 

M 92 - Sep 15, 2020, processed and sharpened

         

M 92 - Sep 15, 2020, manual exposure

 

M 92 - Sep 15, 2020, processed

 

M 92 - Sep 15, 2020, processed and sharpened

         

M 92 - Sep 15, 2020, manual exposure

 

M 92 - Sep 15, 2020, processed

 

M 92 - Sep 15, 2020, processed and sharpened

         

M 92 - Sep 28, 2020, disturbed by clouds

 

M 92 - Sep 28, 2020, processed

 

M 92 - Sep 28, 2020, processed and sharpened

         

M 92 - Sep 28, 2020, disturbed by clouds

 

M 92 - Sep 28, 2020, processed

 

M 92 - Sep 28, 2020, processed and sharpened

         

M 92 - Jul 18, 2021

 

M 92 - Jul 18, 2021, processed

 

M 92 - Jul 18, 2021, processed and sharpened

         

M 92 - Aug 20, 2021

 

M 92 - Aug 20, 2021, processed

 

M 92 - Aug 20, 2021, processed and sharpened

         

M 92 - Aug 20, 2021

 

M 92 - Aug 20, 2021, processed

 

M 92 - Aug 20, 2021, processed and sharpened

         

M 92 - Oct 16, 2021

 

M 92 - Oct 16, 2021, processed

 

M 92 - Oct 16, 2021, processed and sharpened

        

M 92 - Oct 19, 2021

 

M 92 - Oct 19, 2021, processed

   

eVscope 2

         

M 92 - Aug 21, 2023

 

M 92 - Oct 10, 2023, 5 min

 

M 92 - Dec 18, 2023, 3 min

      

M 92 - Aug 21, 2023, photo on top processed

 

M 92 - Oct 10, 2023, photo on top processed

 

M 92 - Dec 18, 2023, photo on top processed

Vespera

M 92, Jul 29, 2022 - original (29 frames = 290s)

Vespera Pro

    

M 92, Jun 4, 2024 - 2000p (90 frames = 900s)

 

M 92, Jun 4, 2024 - 2000p (92 frames = 900s), processed

 

M 92, Jun 4, 2024 - 1800p (90 Frames = 900s), 1:1 section

 

M 92, Jun 4, 2024 - 1800p (90 Frames = 900s), 1:1 section, processed