The Cassini-Huygens mission to Saturn provided a close-up study of the gas giant planet, as
well as its rings, moons, and magnetosphere. The Cassini spacecraft arrived at Saturn in …

Here we review the origin, evolution, and compositional properties of Saturn's ring moons.
This class of eleven small satellites includes objects orbiting near the outer edge of the main …

We present an improved model for interplanetary dust grain fluxes in the outer Solar System
constrained by in situ dust density observations. A dynamical dust grain tracing code is used …

We assess the prospect of using ring seismology to probe the interiors of the ice giants
Uranus and Neptune. We do this by calculating normal-mode spectra for different interior …

INTRODUCTION Saturn's main ring system is associated with a family of small moons. Pan
and Daphnis orbit within the A-ring's Encke Gap and Keeler Gap, respectively, whereas …

Airless bodies are directly exposed to ambient plasma and meteoroid fluxes, making them
characteristically different from bodies whose dense atmospheres protect their surfaces from …

The origin and long-term evolution of Saturn's rings is still an unsolved problem in modern
planetary science. In this chapter we review the current state of our knowledge on this long …

INTRODUCTION Most magnetized planets are known to possess radiation belts, where high-
energy charged particles are trapped in large numbers. The possibility that a radiation belt …

More than a dozen small (< 150 km mean radius) satellites occupy distinct dynamical
positions extending from within Saturn's classical rings to the orbit of Dione. The Cassini …

In the caviar software package, a standard tool for astrometry of images from the Cassini
imaging science subsystem (ISS), Gaussian fitting is used to measure the centre of point-like …