• Comet 220P/McNaught (07-September-2026)

    Although comet C220P/McNaught is dimming, I continue my observations with the Vespera telescopes. The Manual Targets in Singularity were updated with the new coordinates for the comet obtained from Stellarium (RA/Dec: 03h 24m 31s; +08° 28′ 13″). Based on my previous study (20261006) I configured the object type as ‘Cluster’. Because the comet is getting dimmer, I increased the gain to 24 dB for Vespera 1, Vespera 2, and Vespera Passengers; and to 20 dB for Vespera 3, Vespera Pro 1, and Vespera Pro2.

    The comet is still visible to the telescopes. The tail, still > 0.5° long is fading. According to the Comet Observers Database (COBS) the visual magnitude of the comet was 11.2 for the night. It will be interesting to see how much longer I will be able to observe comet 220P/McNaught with the Vespera telescopes.

    The following slideshows include the straight out of the telescope (SOOT) images and images processed with PixInsight. For scale, I’ve included annotated and cropped images (1.0° FOV width). All of the images including the 16-bit RAW/TIFF files are available on my PhotoShelter site (20260907). Click on the i below the slideshow to view the image captions.


    Vespera 1 Telescope


    Vespera Passengers Telescope


    Vespera 2 Telescope


    Vespera 3 Telescope


    Vespera Pro 1A Telescope


    Vespera Pro 1B Telescope


    Vespera Pro 2 Telescope


    Links to my previous observations of comet 220P/McNaught: 20260606, 20260609, 20260616, 20260810, 20260811, 20260815, 20260816, 20260819, 20260820, 20260824, 20260825, 20260826, 20260829, 20260830, 20260906


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  • Comet 220P/McNaught (06-September-2026)

    After nearly a week of rain and cloudy nights the ClearNightSky forecast looked good for continuing the observation of comet C220P/McNaught. The Waning Crescent moon is dimmer (~24% illuminated) than the last observation. I updated the manual target coordinates (RA/Dec: 03h 23m 35s; +08° 33′ 22″) for the comet in Singularity and started an overnight observation plan.

    The comet is dimming, and the tail is less visible. According to the Comet Observers Database (COBS) the visual magnitude of the comet was 11.0 for the night.

    The following slideshows include the straight out of the telescope (SOOT) images and images processed with PixInsight. For scale, I’ve included annotated and cropped images (1.0° FOV width). All of the images including the 16-bit RAW/TIFF files are available on my PhotoShelter site (20260906). Click on the i below the slideshow to view the captions with information about each image.


    Vespera 1 Telescope


    Vespera Passengers Telescope


    Vespera 2 Telescope


    Vespera 3 Telescope


    Vespera Pro 1A Telescope


    Vespera Pro 1B Telescope


    Vespera Pro 2 Telescope


    Links to my previous observations of comet 220P/McNaught: 20260606, 20260609, 20260616, 20260810, 20260811, 20260815, 20260816, 20260819, 20260820, 20260824, 20260825, 20260826, 20260829, 20260830


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  • Optimization Viewing Comet 220P/McNaught with Vespera Telescopes – Part 4

    The ClearNightSky forecast showed clear skies predicted for the whole night. I wanted to repeat the Part 3 results making observation of comet 220P/McNaught using the three target types (nebula, galaxy, or cluster). This time with the gain set to 15 dB or 20 dB. Mainly to confirm that “cluster” is the best manual target choice to minimize the issue of the center background gradient. It has been six nights since the last good observations and according to the Comet Observers Database (COBS) the visual magnitude of the comet dimmed to +11.0.

    The observations from the Vespera 3, Vespera Pro 1, and Vespera Pro 2 telescopes are shown below. These are the unedited, “straight out of the telescope” (SOOT) JPG images. Click on the i below the slideshow to see the caption with the Manual Target parameters.

    The “cluster” manual target observation type remains the best, with galaxy coming a close second. The comet and tail are more difficult to view in the images with “nebula” as the target type.


    Vespera 3 Telescope


    Vespera Pro 1A Telescope


    Vespera Pro 1B Telescope


    Vespera Pro 2 Telescope



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  • Comet 220P/McNaught (30-August-2026)

    The ClearNightSky forecast didn’t look promising but showed some periods that the sky might be clear. I set up the telescopes continuing for more comet  Comet 220P/McNaught observations. I also wanted to further test the Manual Target object modes (nebula, galaxy, or cluster). The observing conditions ended up being marginal. The comet appeared fainter, and the tail shorter than the previous night. According to the Comet Observers Database (COBS) the visual magnitude was +10.3 (same as the previous night).

    The following slideshows include the straight out of the telescope (SOOT) images and images processed with PixInsight. For scale, I’ve included annotated and cropped images (0.5° and 1.0° FOV width). All of the images including the 16-bit RAW/TIFF files are available on my PhotoShelter site (20260830). Click on the i below the slideshow to view the image captions.


    Vespera 1 Telescope


    Vespera Passengers Telescope


    Vespera 2 Telescope


    Vespera 3 Telescope


    Vespera Pro 1A Telescope


    Vespera Pro 1B Telescope


    Vespera Pro 2 Telescope


    Links to my previous observations of comet 220P/McNaught: 20260606, 20260609, 20260616, 20260810, 20260811, 20260815, 20260816, 20260819, 20260820, 20260824, 20260825, 20260826, 20260829


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  • Optimization Viewing Comet 220P/McNaught with Vespera Telescopes – Part 3

    Continuation of the bright center background gradient investigation and optimization of comet 220P/McNaught observations on Vespera telescopes. When setting up a manual target in Singularity there are three target types (nebula, galaxy, and cluster) for objects that the telescope will stack images. Up to this point, I use nebula as the target type. It is first in the list when selecting the type. For tonight’s observations I created manual targets using nebula, galaxy, or cluster, with either the default or increased gain.

    The results are shown in the unedited, “straight out of the telescope” (SOOT) JPG images below and are available in my PhotoShelter gallery. Click on the i below the slideshow to see the caption with the Manual Target parameters.

    The “cluster” target type is the clear winner, with galaxy coming in second. Other than the Vespera 1 telescope, observations with the nebula mode have the center background gradient problem.


    Vespera 1 Telescope


    Vespera Passengers Telescope


    Vespera 2 Telescope


    Vespera 3 Telescope


    Vespera Pro 1A Telescope


    Vespera Pro 1B Telescope


    Vespera Pro 2 Telescope



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  • Comet 220P/McNaught (29-August-2026)

    After a couple of cloudy nights the ClearNightSky forecast looked good for continuing the observation of comet C220P/McNaught. However, the Waning Gibbous moon is bright (~98% illuminated) making the observation more challenging. I updated the manual target coordinates (RA/Dec: 03h 15m 18s; +09° 05′ 24″) for the comet in Singularity and started an overnight observation plan.

    The comet is fainter, and the tail is more than 0.5° long. According to the Comet Observers Database (COBS) the visual magnitude of the comet continues to dim and was 10.3 for the night.

    The following slideshows include the straight out of the telescope (SOOT) images and images processed with PixInsight. For scale, I’ve included annotated and cropped images (1.0° FOV width). All of the images including the 16-bit RAW/TIFF files are available on my PhotoShelter site (20260826). Click on the i below the slideshow to view the captions with information about each image.


    Vespera 1 Telescope


    Vespera Passengers Telescope


    Vespera 2 Telescope


    Vespera 3 Telescope


    Vespera Pro 1A Telescope


    Vespera Pro 1B Telescope


    Vespera Pro 2 Telescope


    Links to my previous observations of comet 220P/McNaught: 20260606, 20260609, 20260616, 20260810, 20260811, 20260815, 20260816, 20260819, 20260820, 20260824, 20260825, 20260826,


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  • Comet 220P/McNaught (26-August-2026)

    The continuing observations of comet C220P/McNaught with my Vespera telescopes. Third night in a row that the night sky remained clear which has been unusual this spring and summer. I updated the manual target coordinates (RA/Dec: 03h 11m 33s; +09° 14′ 28″) for the comet in Singularity and started overnight observation plans for the Vespera telescopes.

    The head of the comet is green, and the tail remains nearly 1° long. According to the Comet Observers Database (COBS) the visual magnitude of the comet continues to dim and was 10.1 for the night.

    The following slideshows include the straight out of the telescope (SOOT) images and images processed with PixInsight. For scale, I’ve included annotated and cropped images (1.0° FOV width). All of the images including the 16-bit RAW/TIFF files are available on my PhotoShelter site (20260826). Click on the i below the slideshow to view the captions with information about each image.


    Vespera 1 Telescope


    Vespera Passengers Telescope


    Vespera 2 Telescope


    Vespera 3 Telescope


    Vespera Pro 1A Telescope


    Vespera Pro 1B Telescope


    Vespera Pro 2 Telescope


    Links to my previous observations of comet 220P/McNaught: 20260606, 20260609, 20260616, 20260810, 20260811, 20260815, 20260816, 20260819, 20260820, 20260824, 20260825


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  • Comet 220P/McNaught (25-August-2026)

    The continuing observations of comet C220P/McNaught with my Vespera telescopes. I updated the manual target coordinates (RA/Dec: 03h 10m 15s; +09° 17′ 05″) for the comet in Singularity and started overnight observation plans for the Vespera telescopes.

    The head of the comet is green, and the tail is nearly 1° long. According to the Comet Observers Database (COBS) the visual magnitude of the comet was 10.0 for the night.

    The following slideshows include the straight out of the telescope (SOOT) images and images processed with PixInsight or Sky Color Studio. For scale, I’ve included annotated and cropped images (1.0° FOV width). All of the images including the 16-bit RAW/TIFF files are available on my PhotoShelter site (20260825). Click on the i below the slideshow to view the image captions.


    Vespera 1 Telescope


    Vespera Passengers Telescope


    Vespera 2 Telescope


    Vespera 3 Telescope


    Vespera Pro 1A Telescope


    Vespera Pro 1B Telescope


    Vespera Pro 2 Telescope


    Links to my previous observations of comet 220P/McNaught: 20260606, 20260609, 20260616, 20260810, 20260811, 20260815, 20260816, 20260819, 20260820, 20260824


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  • Comet 220P/McNaught (24-August-2026)

    The continuing observations of comet C220P/McNaught with my Vespera telescopes. After several cloudy days and nights, the ClearNightSky forecast looked good for two or three nights. I updated the manual target coordinates (RA/Dec: 03h 09m 01s; +09° 19′ 20″) for the comet in Singularity and started overnight observation plans for the Vespera telescopes.

    The head of the comet is green, and the tail is nearly 1° long. According to the Comet Observers Database (COBS) the visual magnitude of the comet was 9.9 for the night.

    The following slideshows include the straight out of the telescope (SOOT) images and images processed with PixInsight . For scale, I’ve included annotated and cropped images (0.5° and 1.0° FOV width). All of the images including the 16-bit RAW/TIFF files are available on my PhotoShelter site (20260824). Click on the i below the slideshow to view the image captions.


    Vespera 1 Telescope


    Vespera Passengers Telescope


    Vespera 2 Telescope


    Vespera 3 Telescope


    Vespera Pro 1A Telescope


    Vespera Pro 1B Telescope


    Vespera Pro 2 Telescope


    Links to my previous observations of comet 220P/McNaught: 20260606, 20260609, 20260616, 20260810, 20260811, 20260815, 20260816, 20260819, 20260820


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  • Optimization Viewing Comet 220P/McNaught with Vespera Telescopes – Part 2

    Continuation of the bright center background gradient investigation and optimization of comet 220P/McNaught observations on Vespera telescopes. The Vespera telescopes have a Mosaic mode whereby images greater than the sensor size can be created. It does this by taking a series of overlapping images and combining them into a single larger image. For this night’s observations I had the telescopes do a regular (non-mosaic) observation, the default size mosaic, and the minimum size mosaic observation of comet 220P/McNaught. The default mosaic size is different for each type of Vespera telescope, and the minimum size is the field of view (FOV) area of the sensor.

    The results are shown in the unedited, “straight out of the telescope” (SOOT) JPG images below and are available in my PhotoShelter gallery. Click on the i below the slideshow to see the caption with the Manual Target parameters.

    Again, the center gradient is not present for the Vespera 1 images but is visible with the other telescopes. I kept the total observation time around 15-20 minutes to minimize the motion of the comet relative to the stationary stars. This is much less than the recommended 2+ hours and is not enough time to complete the mosaic. The background gradient at the overlaps is not smooth. Next time I will investigate the different object types (nebula, galaxy, and cluster).


    Vespera 1 Telescope


    Vespera Passengers Telescope


    Vespera 2 Telescope


    Vespera 3 Telescope


    Vespera Pro 1A Telescope


    Vespera Pro 1B Telescope


    Vespera Pro 2 Telescope



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