There are still many open questions regarding the nature of Uranus and Neptune, the
outermost planets in the Solar System. In this review we summarize the current-knowledge …

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

Materials at high pressures and temperatures are of great interest for planetary science and
astrophysics, warm dense-matter physics and inertial confinement fusion research …

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 …

Thousands of exoplanets have now been discovered with a huge range of masses, sizes
and orbits: from rocky Earth-like planets to large gas giants grazing the surface of their host …

The Juno spacecraft has measured Jupiter's low‐order, even gravitational moments, J2–J8,
to an unprecedented precision, providing important constraints on the density profile and …

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 …

Jupiter's atmosphere is rotating differentially, with zones and belts rotating at speeds that
differ by up to 100 metres per second. Whether this is also true of the gas giant's interior has …

A primary goal of exoplanet characterization is to use a planet's current composition to
understand how that planet formed. For example, the C/O ratio has long been recognized as …

Atmospheric characterization through spectroscopic analysis, an essential tool of modern
exoplanet science, can benefit significantly from the context provided by the interior structure …