Cockermouth Astronomical Society

Cockermouth Astronomical Society A friendly local society for everyone interested in astronomy and space exploration We hold regular meeting and observing events in Cockermouth.

For more information check out our website www.cockermouthastronomy.co.uk

20/05/2026

Next meeting:
Tuesday 26th May 7:30 pm
Quaker Meeting House, Kirkgate, Cockermouth
Agenda:
1. AGM
2. June "night" sky - Will McAllister
Coffee break
3. News round up - Bill McAllister
4. AOB. See less

25/04/2026

Next meeting:
Tuesday 28th April 7:30 pm
Quaker Meeting House, Kirkgate, Cockermouth
Agenda:
1. May "night" sky - Will McAllister
Coffee break
2. News round up - Bill McAllister
3. AOB.

30/03/2026

Next meeting:
Tuesday 31st March 7:30 pm
Quaker Meeting House, Kirkgate, Cockermouth
Agenda:
1. April "night" sky - Will McAllister
Coffee break
2. News round up - Bill McAllister
3. M42 image; AOB.

I have not done any Astronomical Imaging for a few months.  However, over the Christmas period recently I did gather dat...
21/03/2026

I have not done any Astronomical Imaging for a few months. However, over the Christmas period recently I did gather data on this Deep Space Object, namely The M42 Orion Nebula.

This diffuse nebula is very close, sitting at only 1344 Light Years from Earth, in the constellation of Orion. It is an easy target to capture, but you need to use different exposure lengths in order to attempt to preserve data of the Core. If not you will waste a lot of time and the core will be blown out. I took test exposures before capturing, ranging from 1 second up to 10 seconds and then 120 seconds and finally 300 seconds. It took a couple of weeks to collect all the narrowband data sets.

The nebula is a stellar nursery and there are four trapezium stars present in the core and they are the reason for taking different length exposures.

Finally on Thursday, whilst at home with Shirley I sought to process the data.

The image is my first draft of the Nebula and I have not looked at the Orion Nebula in almost 5 years. I do not think it is too bad.

Capturing Telescope: Williams Optics ZS 73 mm refractor.
Guiding Telescope: Ascension 80 mm Triplet Refractor.
Imaging Camera: Atik 460 Ex Mono
Guiding Camera: Atik 314L+
Mount: Skywatcher NEQ6
Filters: Badder Hydrogen Alpha, Oxygen III & Sulphur II.

The Image was processed using Pixinsight.

24/02/2026

Next meeting:
Tuesday 24th February 7:30 pm
Quaker Meeting House, Kirkgate, Cockermouth
Agenda:
1. News round up - Bill McAllister
Coffee break
2. October "night" sky - Will McAllister
3. AOB.

26/01/2026

Next meeting:
Tuesday 27th January 7:30 pm
Quaker Meeting House, Kirkgate, Cockermouth
Agenda:
1. News round up - Bill McAllister
2. October "night" sky - Will McAllister
Coffee break
3. Vera C Rubin Observatory update.

25/11/2025

Next meeting:
Tuesday 25th November 7:30 pm
Quaker Meeting House, Kirkgate, Cockermouth
Agenda:
1. News round up - Bill McAllister
2. October "night" sky - Will McAllister
Coffee break
3. Any other business.

NOTE: This will be the lastr meeting of 2025, as we don't meet in December.

13/10/2025

Rho Ophiuchi and the Antares region in Scorpius. Taken from Boa Vista in Cape Verde, 22nd Sept 2025. Seeing conditions were quite poor due to high atmospheric cloud. But the skies are so dark! The location measured 21.95 SQM, which is Bortle 1 or 2. Some parts of the island have absolutely zero ligh...

NGC7000 Nebula The image is part of the North America Nebula (NGC 7000).  It is an is an emission nebula in the constell...
04/10/2025

NGC7000 Nebula
The image is part of the North America Nebula (NGC 7000). It is an is an emission nebula in the constellation Cygnus and is close to the bright star Deneb. The nebula is very large, approximately 140 light years in width and about 90 light years from top to bottom. The actual distance has been debated but is now said to be 2590 light years from us.
I started collecting data for this target on 16th May 2025, but did not finish until mid July, due to the weather and poor conditions.
I abandoned on several occasions, but managed to get there in the end.
There is a vast amount of activity going on in this image. Dust regions are very visible, along with lots of nebulosity and ionisation. The stars are not as large as I expected and I cannot see any red giants in there which may indicate this lot is not that old. There is an open cluster visible to the bottom of the image.
Overall not so bad. What was pleasing was the ability to go back and go straight onto the target with out loss of data. How you learn over the years.
The image consists of just short of ten hours in Hydrogen, Oxygen and Sulphur. These are narrowband filters. I would have taken more but I could see the optics dewing up.
Equipment:
Telescope: Williams Optics ZS73mm Refractor
Camera: Atik 460Ex Mono
Filter Wheel: Atik Atik EFW2
Guide scope: Ascension 80mm Refractor
Guide Camera: Atik 314L+
Mount Skywatcher NEQ6

The image is the Western Veil nebula, which forms part of the Cygnus loop. The Nebula is catalogued as NGC6960 and has t...
04/10/2025

The image is the Western Veil nebula, which forms part of the Cygnus loop. The Nebula is catalogued as NGC6960 and has the name of the Witches Broom. This object is directly above us now situated in the Constellation of Cygnus at a distance of 2400 light years.
I started collecting data for this target on 16th August 2025 and completed the captures on 23 September 2025. This image consists of exactly 10 hours data collected over three separate nights.
What you can see are the remnants of a massive blue-white giant star (bigger than the Sun) that exploded 8000 years ago. For a period, the explosion would have been very luminous and visible during the daytime on Earth.
The nebula's intricate, thread-like filaments consist of heated and ionised gas and dust, primarily oxygen, hydrogen, and sulphur.
The glowing filaments are shockwaves from the supernova moving through space at speeds of 1.5 million kilometres per hour. The nebula continues to be expanding out into space today.
The bright star 52 Cygni at the bottom appears to be part of the Western Veil but is really a foreground star and unrelated to the nebula.

Image by Dennis Kelly

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