Hot Jupiters were the first exoplanets to be discovered around main sequence stars and
astonished us with their close-in orbits. They are a prime example of how exoplanets have …

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 …

Constraining planet formation based on the atmospheric composition of exoplanets is a
fundamental goal of the exoplanet community. Existing studies commonly try to constrain …

The abundance of refractory elements in giant planets can provide key insights into their
formation histories. Owing to the low temperatures of the Solar System giants, refractory …

The masses and radii of exoplanets are fundamental quantities needed for their
characterisation. Studying the different populations of exoplanets is important for …

Our understanding of planet formation has been rapidly evolving in recent years. The
classical planet formation theory, developed when the only known planetary system was our …

INTRODUCTION The interior structure of Saturn, the depth of its winds, and the mass and
age of its rings have been open questions in planetary science. The mass distribution inside …

The depth to which Jupiter's observed east–west jet streams extend has been a long-
standing question,. Resolving this puzzle has been a primary goal for the Juno spacecraft …

The best constraints on the internal structures of giant planets have historically originated
from measurements of their gravity fields,–. These data are inherently mostly sensitive to a …

Current theories of planetary evolution predict that infant giant planets have large radii and
very low densities before they slowly contract to reach their final size after about several …