Here's what I'm talking about:
[youtube]sR2296df-bc[/youtube]
I personally wouldn't care about any sort of design realism. Just give me a crust and some landscape/atmosphere on top, and I'm happy.
A Dyson sphere.





Sure it would be very, very unlikely, but i'm saying if a star system had over one octillion humungous asteroids, and they're all very close together then they would collide because of they're gravity right? And so they would make an asteroid belt that is all one peace. also dark nebulae are the ones that don't let light get through, otherwise we wouldn't be seeing the orion nebula because starlight wasn't getting through, some nebulae reflect but that's another story. I wish that I could show you a video or something for people to understand what i'm saying. :) (PS) Your second paragraph says that "gravity pulls things into spheres" witch is not true because otherwise galaxies would be spheres.They are not possible in nature (maybe artificially, but that raises other questions). We never observe them in planet-forming simulations, even if the mass of the nebula was very high.
The reason is that gravity acts to pull things into spheres. Gravity cannot act to compress things into a solid ring like a ringworld. If you have a disk filled with a high density of planets or protoplanets, then very quickly they will collide and form one or a few massive planets, while also scattering much of the other material away.
All nebulae that are forming stars with planets are opaque to visible light by the way. Astronomical observations of star forming regions must use infrared to peer through the dust.

We're talking about solid objects formed from gravitational collapse. Galaxies are not solid, nor collapsed fully (if they were they would be black holes).

I get it now, Thanks Watsisname!Your scenario would result in a planet (or a few). Any part of the disk that is denser than the surroundings -- even slightly -- will pull more material into it from all sides. Or even by random chance, some asteroids will clump into a more massive one than average, resulting in a similar instability. Rather than forming a solid ring, the disk would fragment into one or more protoplanets that sweep up or scatter away the rest of the material. Basically this is the planet formation process, though starting from asteroids. By increasing the mass of the disk you just make the process faster.
The Orion Nebula contains many stages of star formation, and it is an emission nebula because it has already formed a number of stars which have ionized the surrounding gas. There are also some parts of it which are currently forming planetary systems (proplyds).
If you're interested in what collapsing molecular clouds look like when they are about to form stars inside them, they are opaque, especially in their cores where the protostars are forming. We cannot observe all stages of star formation in visible light.
We're talking about solid objects formed from gravitational collapse. Galaxies are not solid, nor collapsed fully (if they were they would be black holes).
Gravitational collapse forms disks when the particles have too much angular momentum to collapse further, and also are able to collide and settle into a preferred plane.



