Either way, very cool, that helps getting the eyes up for the galaxies scattered in the picture.
Zooming in all the way, the pure "black" areas between stars also seem to have a fair bit of sensor noise that probably plays a part too.
Pixel scale here seems to mean how many arc-seconds a pixel covers. The full moon (or one's thumb at arm's length iirc) substend about 30 arc-minutes (half a degree)
But everything is moving, right? So how could a series of pictures over this long of a time work out to be so clear?
The Earth is rotating, but it's easy to compensate for that so that the stars don't turn into streaks. You just mount the telescope and camera on a motorized mount that turns slowly to counteract the rotation of the Earth. That's cheap and easy to do, so everyone does it unless they specifically want to show off the rotation of the Earth.
Every star in that image has some proper motion, usually dozens or hundreds of km/s, and there's no way to counteract that. For any single exposure that's not large enough velocity to turn the stars into a streak, but it is enough for the stars to be in different positions relative to each other from year to year. Since different panels of the image were captured in different years, the overlaps between those panels won't match perfectly. When stitching the panels together, the photographer will probably have edited the photograph so that each star is taken from only one panel. That will prevent any stars from being cut in half or blurred together from both panels, but there could be stars that moved fast enough to have crossed the boundary between the panels and they could show up in the full image twice. Good luck spotting them though.
The Earth is also moving around the Sun, so there is an additional apparent motion, but it's smaller in magnitude to than the proper motion and won't cause any extra problems.
The gas clouds are also moving. Some of them are expanding, some of them are being pushed by stellar winds, etc. Stars can form in dense clouds, and then the stellar wind from the new star pushes all the remaining dust away to create a bubble. You can see these motions over the course of years, so presumably they caused some minor mismatches between panels that were photographed at different times. Since these features are fuzzy, it's not hard to blend neighboring panels together even when they're taken years apart.
https://www.youtube.com/watch?v=ofCooIkIwvQ is a great explanation with good visuals, and it has photographs taken by the New Horizons probe that directly show stellar parallax when compared with photographs taken at the same time from Earth. Even that is only visible on the nearest stars; none of the other stars in those photographs were close enough to move at all.
The earth is also orbiting the sun pretty fast, but it's my understanding (I'm not an expert) that you don't need to account for error here, since the Orion nebula is so far away. Think about how the sun stays in the same place in the sky even as you're driving fast on the highway. The nebula is unimaginably far away compared to the sun, and relative movement between the earth, the solar system, and Orion are all undetectable at these scales.
I've read that even the Hubble telescope doesn't need to account for parallax error for such far-away objects during long exposures, which can last up to 20 minutes. Maybe someone here on HN can do (or point to) the math for us.
https://www.lesswrong.com/posts/noBKApHwFm8aMuvnw/link-the-g...
I've been doing a lot of landscape astrophotography lately in which I show these objects rising and setting over familiar landscapes to give people an idea of what our human vision is "missing out" on. Here's one of Orion that I took with a 28mm lens -- i.e. pretty wide angle:
And this is to be expected. We are building models to match our observations. "More of the same" is the basic assumption, but it doesn't mean it is true. That's why we experiment: to verify our models and if found wrong, to update them. The more things our model takes into account, the more we can expect it to explain everything, meaning the more we can expect to find "more of the same", but it is never a given.
I mean, we thought we had the universe almost completely figured out in the early 1900s, with just a few details remaining. The "details" turned out to be quantum physics and general relativity...