The Juno mission has revolutionized and challenged our understanding of Jupiter. As Juno
transitioned into its extended mission, we review the major findings of Jupiter's internal …

Radio observations of the atmospheres of the giant planets Jupiter, Saturn, Uranus, and
Neptune have provided invaluable constraints on atmospheric dynamics, physics/chemistry …

The formation history of giant planets inside and outside the Solar System remains
unknown. We suggest that runaway gas accretion is initiated only at a mass of∼ 100 M⊕ …

The disk midplane temperature is potentially affected by the dust traps/rings. The dust
depletion beyond the water snowline will cast a shadow. In this study, we adopt a detailed …

Understanding Jupiter's present‐day interior structure and dynamics is key to constraining
planetary accretion models. In particular, the extent of stable stratification (ie, non …

One of the main objectives of the European Space Agency's Ariel telescope (launch 2029) is
to understand the formation and evolution processes of a large sample of planets in our …

Updated formation and structure models of Jupiter predict a metal-poor envelope. This is at
odds with the two to three times solar metallicity measured by the Galileo probe …

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 …

A key feature of the Galilean satellite system is its monotonic decrease in bulk density with
growing distance from Jupiter, indicating an ice mass fraction that is zero in the innermost …

Planetesimal accretion is a key source for heavy-element enrichment in giant planets. It has
been suggested that Jupiter's enriched envelope is a result of planetesimal accretion during …