Friday, 17 January 2025

My first outing to RAF Harrowbeer at Yelverton

 First visit to UnderSouthWestSkies? Then why not stop off first at the first page to get a flavour of who I am and what I am trying to achieve in this blog: https://undersouthwestskies.blogspot.com/2025/01/welcome-to-my-new-astronomyastrophotogr.html


A new astronomy location for me. Up at Yelverton on the old RAF Harrowbeer airfield right next to Knighthayes tea shop. I tucked into one of the old aircraft standing bays. 

The target for the night was NGC 869, and NGC 884, a double star cluster. My first ever imaging of a double star cluster. Not ideal conditions; a full moon all night and wraith like fog banks just at ground level. No wind and temperatures dropping to around 3C. Some humidity requiring the use of dew bands. 

Throw in wandering sheep, a few boy racers doing the circuit and some 'dodgy looking punters in cars and vans driving around slowly at midnight and it was a more 'edgy', 'uncomfortable' experience compared to my normal experiences down Wembury beach car park and at Wembury Point. 

Equipment for the night was  

  • Canon 800D
  • Zenithstar 61ii with field flattener
  • RVO 32mm F/4 guide scope with ZWO 120mm mini guide cam
  • ASIair mini
  • Skywatcher star adventurer 2i with William Optics wedge base
  • Skywatcher stainless steel tripod
  • Skywatcher 12v 7 amp power bank
  • Various power packs, dew straps and bits a pieces like intervalometer

One new piece of equipment is proving very useful. The 'move-shoot-move' green laser pen which can be attached to the polar-scope eye viewing piece on the SWSA. It makes setting up the tracker in line with Polaris so much quicker. Polar alignment on the ASiair is consequently quicker as well. 

So, data collection? I managed to get 
  • 180 x 60" lights at ISO 800 (three hours worth)
  • 15 each of darks, biases and flats 
For the first time since buying the ASIair mini, I have managed to get to grips with it and the screen shots below show my first night of proper successful guiding. 

There is no declination on the SWSA2i tracker. Getting an average RA of 0.72 - 0.86 is pleasing - guiding was pretty spot on


The time lapse below gives a flavour of the night time conditions.  Over the next few days I will process the data in SIRIL, GraXpert and Affinity Photo and publish the result here as a postscript. 


The full moon proved to be very, very bright on this night and humidity was an issue as plunging temperatures and warmed land led to low level wraith like fog patches appearing and disappearing regularly through the night. 
And an apology. In the video I labelled it  NGC 469 by mistake - sorry! It is of course NGC 869/884 or Caldwell 14

Postscript:
The final image of NGC 869/884

Post editing details: 
  • Stacked and cropped in SIRIL
  • Background extraction in GraXpert
  • Deconvolution, photometric colour calibration, green noise removal in SIRIL
  • Starnett ++ removal in SIRIL
  • Denoising of starmask image in GraXpert
  • GHS and saturation stretches in SIRIL
  • Final edits in RAW camera in Affinity Photo 

NGC 869/884 is a double cluster of stars approximately 7460 light years away from earth. 12.8 million years old (so relatively young) and also known as Caldwell 14, the clusters lie in the constellations of Perseus and Cassiopeia. Visible to the naked eye from dark sky sights when there is no moon, the clusters have a magnitude of 5.3 to 6.1 and each cluster contains 300 to 400 young hot stars.
The clusters were first 'discovered' and described by the Greek astronomer Hipparchus in 130 BCE

Each cluster has around 300+ blue white super giant stars which are moving through space towards Earth at around 80,000 kph. There are also some brighter orange stars within each cluster as well. In mythology, the double cluster represents the jewelled handle of the sword presented to Perseus by the Gods, along with his helmet and shield. 
Space co-ordinates for the double cluster? RA 2hr. 20m  Dec +57deg. 08m
Finally, the double clusters each have a mass >20,000 solar masses. 





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