Tidal interactions between moons and planets can have major effects on the orbits, spins,
and thermal evolution of the moons. In the Saturn system, tidal dissipation in the planet …

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 …

Recent observational constraints on the internal structure of Jupiter and Saturn suggest that
these planets have" fuzzy" cores, ie, gradients of the concentration of heavy elements that …

Tidal interactions between moons and planets can have major effects on the orbits, spins,
and thermal evolution of the moons. In the Saturn system, tidal dissipation in the planet …

Recent measurements of Jupiter's gravitational field (by Juno) and seismology of Saturn's
rings (by Cassini) strongly suggest that both planets have a stably stratified core that still …

Context. The Juno spacecraft has acquired exceptionally precise data on Jupiter's gravity
field, offering invaluable insights into Jupiter's tidal response, interior structure, and …

Recent structure models of Jupiter suggest the existence of an extended region in the deep
interior with a high heavy element abundance, referred to as a dilute core. This finding has …

Linking atmospheric measurements to the bulk planetary composition and ultimately the
planetary origin is a key objective in planetary science. In this work, we identify the cases in …

Context. Rotation is thought to influence the size of convective eddies and the efficiency of
convective energy transport in the deep convection zones of stars. Rotationally constrained …

In this study, we conducted linear instability analysis of penetrative magneto-convection in
rapidly rotating Boussinesq flows within tilted f-planes, under the influence of a uniform …