There are a great many things in astronomy equipment that you can do, but the question is what compromises you face.
The issue that would be most relevant here is the application. For imaging with a small sensor, such as EAA cameras, this would likely be Ok, but only ok. EAA astronomers stack focal reducers on SCTs to achieve this same kind of fast speed.
For visual use though, based on my extensive, but not professional knowledge of SCTs, the issue most likely to be encountered would be aperture loss. To get the focal plane far enough back to use a 2" diagonal, the primary mirror must be moved forward a considerable amount, and when you use a focal reducer, that amount is extreme. This will cause the axial rays to be clipped off either by the secondary mirror baffle or the primary mirror baffle. You would get a wider field, but that field would be greatly dimmed by the aperture loss, and the contrast would suffer significantly due to the larger percentage of obstruction and the smaller aperture. You would get a wider field though (assuming you could reach focus). If you used a 1.25" diagonal, then you would not get a field much wider than if you used a 2" diagonal and eyepiece without the reducer.
Aperture loss is not the end of the world, but by the time you run the numbers, you might find that your 8" SCT is working with 6.5" of aperture, and a transmission of maybe 70%, which means it would not likely be better than a 120mm f/6 refractor as a wide field scope. That being said, if you have the 8", it isn't that much to buy a focal reducer.
There are a great number of things you can do, but that does not mean that they will all work well, so at this point, it simply becomes a question of what compromises the user is comfortable accepting.
Disclaimer: I do not have ray trace data for the model in question, so I am extrapolating from data that I do have and the general behavior of the moving mirror SCT. I may be way off.
Edited by Eddgie, 11 May 2025 - 09:08 AM.