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 …

Uranus and Neptune form a distinct class of planets in our Solar System. Given this fact, and
ubiquity of similar-mass planets in other planetary systems, it is essential to understand their …

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 …

Four spacecraft have been sent to investigate the Saturnian system: Pioneer 11, Voyager 1,
Voyager 2, and Cassini. By analyzing data acquired with these spacecraft together with …

Interior modeling of Jupiter and Saturn has advanced to a state where thousands of models
are generated that cover the uncertainty space of many parameters. This approach …

Radio observations of the atmospheres of the giant planets Jupiter, Saturn, Uranus, and
Neptune have provided invaluable constraints on atmospheric dynamics, physics/chemistry …

We study the relationship of zonal gravity coefficients, J 2n, zonal winds, and axial moment
of inertia (MoI) by constructing models for the interiors of giant planets. We employ the …

Over the past three decades, we have witnessed one of the great revolutions in our
understanding of the cosmos—the dawn of the Exoplanet Era. Where once we knew of just …

Understanding Jupiter's present‐day interior structure and dynamics is key to constraining
planetary accretion models. In particular, the extent of stable stratification (ie, non …

The fluid dynamics planet Saturn gives rise to alternating east–west jet streams, large
cyclonic and anticyclonic vortices, and a dipole-dominant magnetic field that is highly …