Dramatic Cassini images of Saturn’s diaphanous G and E rings are [link {2096}]yielding new clues[/link] about their structure and formation, namely that Enceladus' geysers are the main supply for the E ring, and that a ring arc, orbiting on the inner edge of the G ring, is of the type found orbiting the planet Neptune.

		Jul 5, 2006:	Double-Banded E Ring - Dramatic edge-on Cassini views of Saturn’s E ring, like these side-by-side images, reveal for the first time a double-banded structure similar to that of Jupiter’s gossamer ring and to the bands of dust found within the Sun’s asteroid belt.
		Jul 5, 2006:	Persistent Arc - This movie shows the bright G ring arc flashing around the inner edge of Saturn’s G ring, a tenuous ring outside the main ring system.