Billybob: "Thats a good idea, and shouldnt be too hard because there arre already like 5 different star textures, right?"
- Thanks.
Are there?
chris: "It would be simple to do . . . but is it really worth it? To a nearby (~ 1 au distant) observer, pretty much all stars would look like blazing bright featureless discs, probably with some variation in hue depending on temperature."
- Hm, in artwork you routinely see a lot of difference between stars but maybe that's just poetic license without any foundation in reality?
"Observed through a filter, there might be some more interesting differences . . ."
- Let's suggest that filters are standard issue on our starships!
"Convection occurs throughout the interior of late M stars and not at all in O and B stars. This would presumably make the surfaces of the stars look very different (again, through a filter)..."
- Yes, yes, yes.
"...but don't know exactly what features you could expect to see."
- Neither do I. At least not at this stage. Just thought that red supergiants probably woud have quite low density outer gas layers with discernable hot center area, compared to MS M-stars which would be compact little rascals. That lower range MS M-stars would just not glow with a dimmer light but have kind of more dark streaks on their surfaces (even though I just suggested only one skin for all MS M-stars). That there ought to be a substantial difference in the impression of a white A star compared to a white dwarf like Kapteyn's Star, although to be honest I really don't know in what way.
I do understand however that if most stars look quite alike, then there is little reason for the proposed modifications. Besides, perhaps we simply don't know what different stars actually look like on a closer inspection (filters provided) despite Hubble etc. If we recall, nobody has gone there yet.