While reviewing the solar images with several sunspots, I noticed what appears to be a pair of satellites transiting the solar disk over a 4 second period. I have a composite image and the individual images of the transit. I also found images with silhouettes of birds (Turkey Vultures?) and one with an unidentified object (military jet?). I’ve also added the time-lapse video if you want to look for other objects passing in front of the sun.
Sun with sunspots and the silhouette of a satellite transit. Image taken with a Vaonis Stellina Telescope (400 mm, f/5, 1/4000 sec) with a solar filter. Composite of 4 images processed using Photoshop (Scripts, Statistics, Minimum).Sun with sunspots and the silhouette of a satellite transit. Image taken with a Vaonis Stellina Telescope (400 mm, f/5, 1/4000 sec) with a solar filter. Image 1 of 4. Sun with sunspots and the silhouette of a satellite transit. Image taken with a Vaonis Stellina Telescope (400 mm, f/5, 1/4000 sec) with a solar filter. Image 2 of 4.Sun with sunspots and the silhouette of a satellite transit. Image taken with a Vaonis Stellina Telescope (400 mm, f/5, 1/4000 sec) with a solar filter. Image 3 of 4.Sun with sunspots and the silhouette of a satellite transit. Image taken with a Vaonis Stellina Telescope (400 mm, f/5, 1/4000 sec) with a solar filter. Image 4 of 4.Sun with sunspots and the silhouette of a bird. Image taken with a Vaonis Stellina Telescope (400 mm, f/5, 1/4000 sec) with a solar filter.Sun with sunspots and the silhouette of a bird. Image taken with a Vaonis Stellina Telescope (400 mm, f/5, 1/4000 sec) with a solar filter.Sun with sunspots and the silhouette of an unidentified object. Image taken with a Vaonis Stellina Telescope (400 mm, f/5, 1/4000 sec) with a solar filter.Sun with Sunspots. Time-lapse video (480p, 30p)
Comet C/2023 A3 (Tsuchinshan–ATLAS)
The comet is still visible to the telescopes with an estimated magnitude of +6.8. The tail is fainter and shorter than yesterday. The Vespera II telescope was fitted with a CLS (city light suppression) filter causing the tint to the image. The length of the comet tail can be estimated based on the field of view for the telescope’s digital sensors. Stellina (1.0° x 0.7°), Vespera Classic (1.6° x 0.9°), Vespera Passengers (2.4° x 1.8°), Vespera II (2.5° x 1.4°), 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).
Comet C/2023 A3 (Tsuchinshan–ATLAS). Composite of 30 images taken with a Vaonis Stellina Telescope (400 mm, f/5, 30 x 10 sec).Comet C/2023 A3 (Tsuchinshan–ATLAS). Composite of 30 images taken with a Vaonis Vespera Classic Telescope (200 mm, f/4, 30 x 10 sec).Comet C/2023 A3 (Tsuchinshan–ATLAS). Composite of 30 images taken with a Vaonis Vespera Passengers Telescope (200 mm, f/4, 30 x 10 sec).Comet C/2023 A3 (Tsuchinshan–ATLAS). Composite of 30 images taken with a Vaonis Vespera II Telescope (250 mm, f/5, 30 x 10 sec) using a CLS (city light suppression) filter.Comet C/2023 A3 (Tsuchinshan–ATLAS). Composite of 30 images taken with a Vaonis Vespera-Pro Telescope (250 mm, f/5, 30 x 10 sec).
