Kevin R. Grazier

TL;DR: Observations of Titan from the imaging science experiment onboard the Cassini spacecraft reveal intricate surface albedo features that suggest aeolian, tectonic and fluvial processes, and imply that substantial surface modification has occurred over Titan's history.

TL;DR: Images acquired of Saturn's rings and small moons by the Cassini Imaging Science Subsystem have produced many new findings, including new saturnian moons; refined orbits of new and previously known moons; ring particle albedos in select ring regions; and never-before-seen phenomena within the rings.

TL;DR: The Cassini Imaging Science Subsystem acquired high-resolution imaging data on the outer Saturnian moon, Phoebe, during Cassini's closeFlyby on 11 June 2004 and on Iapetus during a flyby on 31 December 2004.

TL;DR: From analysis of cloud motions through early October 2004, vertical wind shear in Saturn's equatorial jet and a maximum wind speed of ∼375 meters per second are reported, a value that differs from both Hubble Space Telescope and Voyager values.

TL;DR: Weibel et al. as discussed by the authors investigated the existence and importance of stable niches in the Jupiter/Saturn zone using highly accurate numerical techniques based on high-order optimized multistep integration schemes coupled to roundoff error minimizing methods.