Comet 220P/McNaught is now post-perihelion (14-June-2026) and is still visible with my Vespera 3 telescope. I am now able to observe the comet without the trees being in the way. I updated the manual target for the Vespera 3 telescope with the new coordinates for the comet from Stellarium (RA/Dec: 00h40m08s; 04°00’15”). The observation was started at 03:29 and allowed continue until 04:00. The sky gets bright really early this time of the year — it is only a few days before the summer solstice.
I processed the composite 188 frame exposure (1880 sec) TIFF file with PixInsight (AutomaticBackgroundExtractor, SpectrophotometricColorCorrector, NoiseXterminator). When processing the image with PixInsight, AutomaticBackgroundExtractor did a better job than GradientCorrection for flattening the background. Ultimately, I needed to crop the image. The brightness in the corner of the full image is probably due to the early dawn. The straight out of the telescope (SOOF) JPG and 16-bit RAW/TIFF images are available on my PhotoShelter site (20260616).
Vespera 3



The comet is very faint, and the tail is barely visible. Dimmer than on 06-June and 09-June. The estimated magnitude is 12.4. At this point the comet is 224 M km (1.5 AU) from earth. It will be a little over 5 years before it returns.





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