The Juno spacecraft has been collecting data to shed light on the planet's origin and
characterize its interior structure. The onboard gravity science experiment based on X-band …

Giant planets acquire gas, ices and rocks during the early formation stages of planetary
systems and thus inform us on the formation process itself. Proceeding from inside out …

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 …

The Juno orbiter has continued to collect data on Jupiter's gravity field with unprecedented
precision since 2016, recently reporting a nonhydrostatic component in the tidal response of …

Normal mode oscillations in Saturn excite density and bending waves in the C ring,
providing a valuable window into the planet's interior. Saturn's fundamental modes (f …

Normal mode seismology is a promising means of measuring rotation in gas giant interiors,
and ring seismology presents a singular opportunity to do so at Saturn. We calculate …

The next phase in the robotic exploration of the Saturnian system will target unresolved
questions about the gas giant's atmosphere, interior, magnetosphere, and rings that were …

Saturn's C ring contains multiple structures that appear to be density waves driven by time-
variable anomalies in the planet's gravitational field. Semiempirical extensions of density …

The Cassini spacecraft performed several flybys of Saturn's largest moon, Titan, collecting
valuable data. During several passes, altimetric data were acquired. Here, we focus on …

Abstract The most recent Planetary Science and Astrobiology Decadal Survey has proposed
Uranus as the target for NASA's next large-scale mission. The interior structure and …