Groundbased and spacecraft telescopic observations, combined with an intensive modeling
effort, have greatly enhanced our understanding of hot giant planets and brown dwarfs over …

An accurate description of turbulent core convection is necessary in order to build robust
models of planetary core processes. Towards this end, we focus here on the physics of …

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 giant impact hypothesis remains the leading theory for lunar origin. However, current
models struggle to explain the Moon's composition and isotopic similarity with Earth. Here …

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 …

We determine basic thermodynamic and transport properties of hydrogen–helium–water
mixtures for the extreme conditions along Jupiter's adiabat via ab initio simulations, which …

The Juno microwave radiometer measured the thermal emission from Jupiter's atmosphere
from the cloud tops at about 1 bar to as deep as a hundred bars of pressure during its first …

The atmospheric dynamics of Jupiter are dominated by strong zonal winds engulfing the
planet. Since the first gravity measurements taken by Juno at Jupiter, the low-degree gravity …

Stellar differential rotation can be separated into two main regimes: solar-like when the
equator rotates faster than the poles and antisolar when the polar regions rotate faster than …

Benchmark solutions for fully nonlinear anelastic compressible convection and dynamo
action in a rotating spherical shell are proposed. Three benchmarks are specified. The first is …