The first telescope is a 60 travel refractor, followed by an 8 inch Newtonian, then a 102 mm refractor, then a 90 mm Mak. Then the C8 SCT. Why this order? It is in order of increasing focal length, which determines the size of the image on the detector. Note: These images are captured using "lucky imaging", the camera takes several hundred images and "stacks" the images to take the best parts of each image, and discards the poor images.

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