The origin and evolution of Saturn's rings is critical to understanding the Saturnian system as
a whole. Here, we discuss the physical and chemical composition of the rings, as a …

On the largest scales Saturn's rings are often thought of as axisymmetric annuli varying only
radially in optical depth with exceptions of spiral waves and eccentric ringlets. But on scales …

One could become an expert on Saturn's iconic rings pretty easily in the early 1970s, as very
little was known about them beyond the distinction between the A, B, and C rings, and the …

Abstract The Cassini Ultraviolet Imaging Spectrograph (UVIS) included a High-Speed
Photometer (HSP), which observed hundreds of stellar occultations by Saturn's ring system …

INTRODUCTION Saturn's rings are an accessible exemplar of astrophysical disk processes
and a delicate tracer of the Saturn system's dynamical processes and history. RATIONALE …

Abstract The Cassini spacecraft's Ultraviolet Imaging Spectrograph (UVIS) includes a high
speed photometer (HSP) that has observed stellar occultations by Saturn's rings with a …

Abstract In 2017, the Cassini mission Grand Finale provided hints at the total mass of
Saturn's ring system, constraining the age of the rings: they could actually be about 200 …

This study is a companion paper to Baillié et al., in which we showed that a past episode of
inward migration of Mimas could have created the Cassini Division. We here investigate the …

Saturn's C ring and Cassini Division share many morphological traits: both contain
numerous opaque, sharp–edged ringlets and gaps, broader low optical depth “background” …

The D68 ringlet is the innermost narrow feature in Saturn's rings. Prior to 2014, the
brightness of this ringlet did not vary much with longitude, but sometime in 2014 or 2015 a …