The 27 satellites of Uranus are enigmatic, with dark surfaces coated by material that could
be rich in organics. Voyager 2 imaged the southern hemispheres of Uranus's five largest" …

We investigated" muted" craters and scarps across Miranda's cratered terrain. The
morphologies of the muted craters are most consistent with modification by regolith …

We summarize the current state of observations of circumplanetary dust populations,
including both dilute and dense rings and tori around the giant planets, ejecta clouds …

Ring arcs are the result of particles in corotation resonances with nearby satellites. Arcs are
present in Saturn and Neptune systems, in Saturn they are also associated with small …

We report the first near-infrared detection of Uranus's tiny moon Mab, the presumed source
of the blue and diffuse μ ring, using the NIRC2 instrument at Keck Observatory. The …

The G ring arc hosts the smallest satellite of Saturn, Aegaeon, observed with a set of images
sent by Cassini spacecraft. Along with Aegaeon, the arc particles are trapped in a 7: 6 …

ABSTRACT The arcs of Neptune–Fraternité, Egalité, Liberté, and Courage–are four
incomplete rings immersed in the Adams ring. A recent confinement model for the arcs …

Small particles in Pluto's environment: effects of the solar radiation pressure | Monthly Notices
of the Royal Astronomical Society | Oxford Academic Skip to Main Content Advertisement …

The distinctive set of Saturnian small satellites, Aegaeon, Methone, Anthe, and Pallene,
constitutes an excellent laboratory to understand the evolution of systems immersed in co …

Here, we report the results of a set of numerical simulations of the system formed by
Neptune, Galatea, dust ring particles, and hypothetical co-orbital satellites. This dynamical …