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 …

Population studies of exoplanets are key to unlocking their statistical properties. So far, the
inferred properties have been mostly limited to planetary, orbital, and stellar parameters …

The composition of giant planets is imprinted by their migration history and the
compositional structure of their hosting disks. Studies in recent literature have investigated …

The characterisation of giant exoplanets is crucial to constrain giant planet formation and
evolution theory and for putting the solar-system's giant planets in perspective. Typically …

Recent observations of extrasolar gas giants suggest super-stellar C/O ratios in planetary
atmospheres, while interior models of observed extrasolar giant planets additionally suggest …

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⊕ …

In the past decade, ALMA observations have revealed that a large fraction of protoplanetary
discs contains rings in the dust continuum. These rings are the locations where pebbles …

Relating planet formation to atmospheric composition has been a long-standing goal of the
planetary science community. So far, most modeling studies have focused on predicting the …

Upcoming studies of extrasolar gas giants will give precise insights into the composition of
planetary atmospheres, with the ultimate goal of linking it to the formation history of the …

During their formation, planets form large, hot atmospheres due to the ongoing accretion of
solids. It has been customary to assume that all solids end up at the center, constituting a …