David's Images of the Day Photoblog
Views of the sun, moon, and stars
The comet is now high enough just after dusk to view from my patio, so I don’t need to move the Vespera telescopes to the far back section of the yard. It also means I can use the Stellina telescope, which is heavier and requires a sturdier tripod. Note the thin bright streak going back from the head of the comet down the middle of the tail.
Four tripods and four telescopes were set up in the far corner of the back yard to view the comet. The Vespera telescopes weigh 11 lbs (5 kg) which makes them relatively easy to transport and move. I’m not sure why the image from the Vespera Pro telescope was dimmer than the others.
It was another clear night and two tripods and two telescopes were moved to the back section to view the comet. Each night Comet C/2023 A3 (Tsuchinshan–ATLAS) is a little bit higher in the sky but becomes a bit dimmer. The estimated magnitude of the comet was +4.9. The length of the comet tail also decreases every night. The digital sensor field of view for the first image (Vespera Passengers ) with the comet head near the center is 2.4° x 1.8°. For the second image (Vespera II) I was able to get the comet head closer to the bottom. The diagonal field of view for this sensor is 2.5° x 1.4°.
I returned to the far corner of my backyard with a view to the west where Comet C/2023 A3 (Tsuchinshan–ATLAS) was still high enough above the trees be visible just after dusk. The estimated magnitude of the comet was +4.7. I couldn’t see it directly, but easily captured an image with Vespera Pro telescope. This is a composite of 30 stacked 10 second images (300 second exposure).
I found a spot in the far corner of my backyard with a view to the west where Comet C/2023 A3 (Tsuchinshan–ATLAS) was still high enough above the trees after dusk to be visible. The estimated magnitude of the comet was +4.5. To me barely visible to the eye, but easily captured by camera or Vespera telescope.
To observe a comet with the Vespera telescopes, you first need to determine the RA (right ascension) and Dec (declination) coordinates of the comet for your location at the time of the observation. I use Stellarium find this information. The RA/dec data is needed to create a manual observation target in the Singularity application that controls the Vespera telescopes.
The Vespera telescopes weigh about 5 kg (11 lbs) and could easily be carried to the far corner of my backyard and set up on heavy duty camera tripods. The only thing I needed to worry about was a doe that found a hole in my deer fence and was wandering around in the back yard. Once it was dark enough to initialize (automatically align and focus) the Vespera telescopes all I needed to do set it to look for the manual target and start acquiring and stacking images.
The comet was much brighter than the other stars in the field of view. The comet’s tail was longer than the field of view of the telescopes. Vespera Classic (1.6° x 0.9°) and Vespera Pro (1.6° x 1.6°). The jpg images were processed to increase the brightness (Capture One Pro) and reduce the noise (Topaz AI).
