There is a situation in which you can see rings, but requires a very specific scenario.
You start with a binary star system, in which the primary is big enough to go supernova. At a certain time, the primary emits clouds of gases. These clouds are shaped into a thin disk by the gravitational effect of the secondary. This emission ends before the explosion of the primary and the disc becomes a ring of expanding gas. One day, the primary goes boom. A roughly spherical shell of remnants expands at tremendous speed, much higher than the speed with which the previous disc is expanding, so at a certain moment, usually about a decade after the explosion, the supernova shell blasts into the ring and makes it shine... and you have things like
http://en.wikipedia.org/wiki/SN_1987A SN 1987a.
P.S.: add Jar Jar Binks to the reasons for a necktie party....