A brief clearance on 14th January 2010 gave me first light with the new camera and I was able to capture a sequence of Messier 45 - the Pleiades or Seven Sisters. The camera worked well enough, but on processing I found that the field was unevenly focussed. The light of day showed me that the drawtube (which was almost fully retracted to accommodate the AO-8 unit with the William Optics 0.8 reducer/flattener) on my 80 mm refractor was slightly tilted, so one side was approximately 1/2 mm different from the other - enough I presume to affect the focus across the big chip at the f4.8 ratio (f6 scope with 0.8 reducer). I've adjusted the slide bars and it looks better. Next try will tell.... 8 x 5 minute subs, darks and flats applied. Obviously longer subs are required, but weather did not permit. But a reasonably promising start. What is particularly heartening is that I was using the rig on my Autostar DS motor driven EQ3-2 mount. And the AO-8 was able to provide all the correction needed without adjusting the mount at all, indeed it was well within its limits. So an eminently portable system for medium to wide field imaging. No point in supplying a full size image - the quality is very mediocre. |
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Postscript - on 30th January after a prolonged cloudy spell, a clear night, albeit with some high thin cloud. Full Moon, so no chance of nebulosity, but a series of 5 minute exposures proved the focus adjustments to have been successful - much improved across the field, although still not perfect in the corners, but that is probably optical . The moonlight and haze accentuated the vignetting, but no point in applying flats etc. Same setup as before. |
In June, light nights are with me, and unless I go narrowband, only brighter objects are of interest for imaging. So here's one of Corona Borealis from the early hours of 3rd. SBIG ST4000XCM with Tamron 17-50 f2.8 lens unguided on the Gemini mount at 50 mm focal length and f5.6. 10 x 5 minute subs, darks and flats used. Of interest is the large asteroid Pallas at mag 9.0, now gradually fading from a maximum of 8.6 in April. Pure chance that it's in the field - I didn't know until I started playing with a Skymap overlay to work out what was stars and what was noise. In fact nearly all stars, just the odd hot pixel that escaped the dark frame but was then removed. Full Size (810 KB!)
And with added spikes to enhance the brighter stars (they already have diffraction spikes, but quite muted in the original). Full size |
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During a prolonged period of wet and cloudy weather a clear window of a few hours on October 1st gave me an opportunity to image comet 103P Hartley as it passed near NGC281 - the 'Pacman' nebula. This comet was discovered by Malcom Hartley in Australia on March 15, 1986 and has an orbital period of about 6.5 years, so this was its third known pass. Very high in the sky with the tail pointing away, so only the coma visible. Estimated at around 7th magnitude, and was just visible in my 15x50 binoculars. SBIG ST-4000XCM and Canon 400L telephoto lens (400 mm focal length) stopped down to approx. 7.1 using an external mask. 21 sub frames x 3 minutes, stacked using the special comet feature of Deep Sky Stacker. Full size (913KB) There are also animations of the comet head as it moved across the sky during the hour or so of the exposures, cropped from the full size. AVI (748KB) DivX Codec. Or for those who don't have the codec, GIF (3.57 MB) |
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While Earth based telescopes only succeeded in capturing a dot surrounded by a greenish glowing coma, this image was captured by NASA's EPOXI mission between Nov. 3 and 4, 2010, during the spacecraft's flyby of comet Hartley 2. It was captured using the spacecraft's Medium-Resolution Instrument. Image credit: NASA/JPL-Caltech/UMD |
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