Analogous to Earth's water cycle, Titan's methane-based hydrologic cycle supports standing
bodies of liquid and drives processes that result in common morphologic features including …

Abstract The Europa Imaging System (EIS) consists of a Narrow-Angle Camera (NAC) and a
Wide-Angle Camera (WAC) that are designed to work together to address high-priority …

Several planetary satellites apparently have subsurface seas that are of great interest for,
among other reasons, their possible habitability. The geologically diverse saturnian satellite …

Cassini has identified a geologically active province at the south pole of Saturn's moon
Enceladus. In images acquired by the Imaging Science Subsystem (ISS), this region is …

Many white dwarf stars show signs of having accreted smaller bodies, implying that they
may host planetary systems. A small number of these systems contain gaseous debris discs …

We present the first comprehensive examination of the geysering, tidal stresses, and
anomalous thermal emission across the south pole of Enceladus and discuss the …

Titan, the largest moon of Saturn, is the only satellite in the Solar System with a substantial
atmosphere. The atmosphere is poorly understood and obscures the surface, leading to …

We present values for the masses of Saturn and its major satellites, the zonal harmonics in
the spherical harmonic expansion of Saturn's gravitational potential, and the orientation of …

We describe the successful synthesis of modulation-doped silicon nanowires by achieving
pure axial elongation without radial overcoating during the growth process. Scanning gate …

Four spacecraft have been sent to investigate the Saturnian system: Pioneer 11, Voyager 1,
Voyager 2, and Cassini. By analyzing data acquired with these spacecraft together with …