David's Images of the Day Photoblog
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 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).
With the sky clear, I set up the Vespera Observation station with a solar filter during the day to observe sunspots. When I reviewed the images, I found one with a silhouette of a bird (Turkey Vulture?) flying in front of the sun. In the past I have capture images of planes, and sometimes satellites transiting the solar disk. While on Semester at Sea voyages, we had an informal contest to capture images of ships at the horizon passing in front of the sun at sunset (or sunrise).
Once it got dark out, I set up both the Vespera and Stellina observation stations to observe deep sky objects (galaxies, nebulae, star clusters). The Vespera was fitted with a dual band (H-alpha and O-III) filter. The Vespera captured images of NGC 6960: Western Veil Nebula, Witch’s Broom Nebula; IC 1396: Elephant’s Trunk Nebula; and IC 1795: Fish Head Nebula. The final one didn’t go to completion due to condensation on the lens.
For the Stellina, I used the “Plan My Night” option to collect images of Messier 29 Open Cluster (M29, NGC 6913); NGC 6946 (Fireworks Galaxy); NGC 7331 Spiral Galaxy (Caldwel 30); Messier 31 Spiral Galaxy (Andromeda Galaxy, NGC 224); Messier 74 Spiral Galaxy (M74, NGC 628, Phantom Galaxy); Messier 110 Dwarf Elliptical Galaxy (M10, NGC 205); IC 342: The Hidden Galaxy in Camelopardalis. The system was set to collect images for about an hour for each object. For some reason, the telescope did not automatically close at the end of the collection. I am not sure if the external Anker Power USB power supply ran out. The lens was covered with dew. The Stellina system has a lens heater that is supposed to prevent condensation so may be the reason the power bank ran out. The Vespera system does not have the lens heater option installed.
Daily Electric Energy Used (46.5 kWh) from Sense. Daily Solar Electric Energy Produced (51.7 kWh) from Sense. Sunny. Surplus of 5.2 kWh.
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