I'm not the person who created the original ring image, but I thought I'd take some time today to look at Saturn's ring image file /textures/lores/saturn-ring.png
PNG files can contain an alpha (transparency) channel in addition to the main image. I used the netpbm utilities to split the file into separate alpha-channel and image files. As I suspected, the alpha channel in saturn-ring.png is misalighed with the main image. Its Enke's division is displaced radially inward from the Enke's division that's in the image. Other features seem to be similarly offset.
I've created a new png file with its alpha channel identical to the image itself. I'm not sure it's "right", but at least there's only one Enke's division, now
Oh, and before you complain about Pan not being centered in the gap, I checked around on the Web and found that its orbital parameters do indeed correspond to its being near the inner edge of the gap. It turns out that there also are more faint rings both inward and outward from the current ring image that Celestia's using. Creating an entirely new image is more than I'm prepared to do any time soon, though.
What I'd really like to see is a ring png file with an image that corresponds to the rings' measured brightness profile and an alpha channel that corresponds to their transparency. I'm rashly assuming there have been enough stellar occultations by the rings for that to be measured, of course.
Screenshots of Pan in Enke's division along with the revised png file are available on my Web site at
http://www.lns.cornell.edu/~seb/celestia/gallery-001.html#7