Origin of Saturn's E Ring: Self-Sustained, Naturally

Citations Over TimeTop 10% of 1994 papers

Abstract

Saturn's diffuse E ring spans the region between 3 and 8 saturnian radii ( R s ), has its peak brightness near the orbit of the satellite Enceladus (3.95 R s ), and is thought to be composed primarily of icy particles 1.0 ± 0.3 micrometers in radius. Such particles are shown to move periodically along highly elliptical paths that cross the orbits of several saturnian satellites; the resulting energetic collisions of E ring particles with embedded satellites are capable of sustaining the E ring at its current optical depth. With several reasonable assumptions, this model naturally selects Enceladus as the primary source of ring material and may also provide mechanisms that explain the generation of the unusual amount of submicrometer dust in the neighboring F and G rings, the excess of OH molecules observed within the E ring, and the orbital brightness variations of nearby satellites.

Related Papers

• → Sodium salts in E-ring ice grains from an ocean below the surface of Enceladus(2009)577 cited
• → Seasonal variations in Saturn's plasma between the main rings and Enceladus(2012)34 cited
• → Cold cases: What we don't know about Saturn's Moons(2017)6 cited
• → Does Enceladus Govern Magnetospheric Dynamics at Saturn?(2006)31 cited
• → Dusty plasma around Enceladus affects Saturn's magnetosphere(2012)