Recent advances in interplanetary dust modelling provide much improved estimates of the
fluxes of cosmic dust particles into planetary (and lunar) atmospheres throughout the solar …

Abstract ESA's Jupiter Icy Moons Explorer (JUICE) will provide a detailed investigation of the
Jovian system in the 2030s, combining a suite of state-of-the-art instruments with an orbital …

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 …

Ablation of interplanetary dust supplies oxygen to the upper atmospheres of Jupiter, Saturn,
Uranus, and Neptune. Using recent dynamical model predictions for the dust influx rates to …

Molecular species in planetary atmospheres provide key insights into their atmospheric
processes and formation conditions. In recent years, high-resolution Doppler spectroscopy …

Saturn's northern summertime hemisphere was mapped by JWST/Mid‐Infrared Instrument
(4.9–27.9 µm) in November 2022, tracing the seasonal evolution of temperatures, aerosols …

Abstract During the Grand Finale stage of the Cassini mission, organic-rich ring material was
discovered to be flowing into Saturn's equatorial upper atmosphere at a surprisingly large …

The exploration of carbon-to-oxygen ratios has yielded intriguing insights into the
composition of close-in giant exoplanets, giving rise to a distinct classification: carbon-rich …

The study of planets and small bodies within our Solar System is fundamental for
understanding the formation and evolution of the Earth and other planets. Compositional …

Transmission spectroscopy is enabling precise measurements of atmospheric H2O
abundances for numerous giant exoplanets. For hot Jupiters, relating H2O abundances to …