Structure and particle properties of Saturn's E Ring

Astronomy and Astrophysics – Astronomy

Scientific paper

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Particle Size Distribution, Planetary Structure, Saturn Rings, Astronomical Photometry, Charge Coupled Devices, Satellite Imagery, Three Dimensional Models, Voyager Project

Scientific paper

The present systematic reanalysis of a substantial portion of extant photometric data on the Saturn E Ring has calibrated every observation on the basis of a common 3D model. A simple power-law model is found to describe the ring's normal optical depth profile with orbital radius; this trend is departed from, however, near the density peak, where there emerges a 30-percent localized decrease in thickness. No power-law size distribution is found to be compatible with available photometry. The peculiar size distribution points to a ring origin in a process that was not collisional or disruptive.

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