Ultra Deep look at Messier 81 and 82
theuberger.ch
theuberger.ch
- Olaf Stapledon, Star Maker
Not much inspires a sense of meaning in me these days like the sheer scope and scale and depth of creation.
Beautiful work.
By far the greatest thing that improves astrophotography is the ability to collect light for a long time, and this implies tracking the movement of the stars across the sky. I'd say that this is more important than having a telescope. Without it, you're limited to taking pictures short enough that the stars don't move more than a pixel or two in that time, which is typically between a tenth of a second and ten seconds, depending on the zoom level of your lens. However, you can take multiple pictures and combine them. With a tracker, you can easily take exposures that are minutes long.
Lucky imaging is useful for things that are very bright, and it allows you to sharpen up the image. It works for the moon, and the brightest parts of some galaxies or nebulae. But the normal things that make spectacular astrophotography images aren't really helped by it. Mostly, the best thing to make images better is just to collect more light. Lucky imaging is great, but it's a niche.
It does work. I have produced acceptable images of the Andromeda galaxy by using a 150-600mm lens at 150mm on a tripod taking 1.3s exposures. I took 1151 images, which is a total of 24 minutes of light collection, and the image was rather mediocre.
I then make a rudimentary tracker, and took 22 exposures of 6s each, at 600mm, and the results were way better. At 600mm, I would have had to take 0.3s exposures untracked, and it would have been awful. I then bought a proper tracker, and did 254 exposures of 30s each at 600mm, and the result was just so much better.
The problem is that a lot of the pretty stuff we can make pictures of is very dim, so the main thing driving image quality (assuming the optics are OK) is the noise level of those dark pixels.
There are several reasons why it is better to have a physical tracker. One is that the noise from the sensor consists of shot/Poisson noise (from the photons coming in), dark current, and readout noise. If you have very short exposures, then the readout noise dominates. The shot noise is a physical limit - you can't get lower noise than the shot noise for the number of photons that you collect; you can only improve that by collecting more photons. The readout noise is entirely added by the equipment, and you can minimise that by taking longer exposures. The dark current is improved by cooling the sensor down. Other reasons are the data quantity (if you're processing it later or keeping the raw data, as most astrophotographers do), processing time, and wear on the shutter mechanism (if it is mechanical). Also, if you have a reasonably long telescope, if you don't have a tracker then the subject will keep moving out of the frame in less time than you would expect, and you'll have to keep re-pointing the telescope anyway.
Lucky imaging is the opposite - then you do deliberately want to take lots of short exposures to get sharper images, but the trade-off is that the noise is higher, and you really want to have a sensor with an electronic shutter. Short exposures are only suitable when there is something in the frame that is bright enough to register as a reasonably bright few pixels, otherwise there is nothing to align the frames with, and lucky imaging can't work out how sharp each frame is.
OpenSeadragon: An open-source, web-based viewer for high-resolution zoomable images
I love images from astronomy, but I wish it was generally made clearer when color enhancement is and is not used.
https://blogs.nasa.gov/superpressureballoon/2023/04/20/ballo...
Amazing.