A Couple of Globular Clusters (5/15/2021)

Messier 3 and Messier 52 captured in May. Celestron 8 on Celestron AVX mount, Starizona Night Owl, ASI294MC Pro. Exposure 30 x 30s. Guided by Orion Magnificent Mini Autoguider. 

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Messier 3

Messier 52

Ad hoc bonus night

If the NOAA forecast for a dark site is partly cloudy I don't bother planning a DSO imaging mission. However, on the afternoon of this mission I noticed the skies were sunny and cloudless. Upon checking Clear Sky Chart for Harvard MA it was forecasting an above average viewing night. Other than picking a few Galaxy Season targets little planning was needed. The night went well with the images appearing below. Galaxy images were averaged from 15x60s exposure sub frames. Globular clusters were averaged from 25x30s exposure sub frames.

Messier 51 (Whirlpool Galaxy)

 

Messier 64(Black Eye Galaxy)

Messier 3

Messier 53

Messier 85(center) and NGC 4394(lower center)

M86 (low right), M84(upper center),
NGC4402(lower left), NGC4388(right center)

NGC4565

Under a full moon

June 16 was just one day past full moon. Between 10 and 11PM the moon was still low to the southeast which offered a test for using the DSI-2 under fairly adverse conditions. Randolph, MA where I live is already very light polluted with poorly shielded sodium vapor lights. Adding to the challenge, the  local elementary school in whose parking lot I do my local observing has both broadband mercury vapor along with sodium vapor lighting.

Messier 3 just past full moon

After setting up the scope it took longer than usual to iterative align the 127ED because I forgot about the problems posed by using Arcturus or Spica as alignment stars. I need to recompile a list of compatible alignment stars which which differ between 3 and 9 hr away from Polaris in R.A.


I chose M3, which rides high in the sky this time of night to image. The globular cluster was obvious at 1s exposures in focus mode. After  creating a fresh set of darks for the night and merging with my old set of darks I acquired two sets of exposures at 2.8 and 4.0s. The 4.0s set were averaged to produce the final image after some histogram, brightness and contrast tweaking.